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href="//donate.wikimedia.org/wiki/Special:FundraiserRedirector?utm_source=donate&utm_medium=sidebar&utm_campaign=C13_ko.wikipedia.org&uselang=ko" class=""><span>기부</span></a> </li> <li id="pt-createaccount-2" class="user-links-collapsible-item mw-list-item user-links-collapsible-item"><a data-mw="interface" href="/w/index.php?title=%ED%8A%B9%EC%88%98:%EA%B3%84%EC%A0%95%EB%A7%8C%EB%93%A4%EA%B8%B0&returnto=%ED%95%AD%EC%84%B1%EA%B3%84" title="계정을 만들고 로그인하는 것이 좋습니다. 하지만 필수는 아닙니다" class=""><span>계정 만들기</span></a> </li> <li id="pt-login-2" class="user-links-collapsible-item mw-list-item user-links-collapsible-item"><a data-mw="interface" href="/w/index.php?title=%ED%8A%B9%EC%88%98:%EB%A1%9C%EA%B7%B8%EC%9D%B8&returnto=%ED%95%AD%EC%84%B1%EA%B3%84" title="위키백과에 로그인하면 여러가지 편리한 기능을 사용할 수 있습니다. [o]" accesskey="o" class=""><span>로그인</span></a> </li> </ul> </div> </div> </div> <div id="vector-user-links-dropdown" class="vector-dropdown vector-user-menu vector-button-flush-right vector-user-menu-logged-out" title="더 많은 옵션" > <input type="checkbox" id="vector-user-links-dropdown-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-vector-user-links-dropdown" class="vector-dropdown-checkbox " aria-label="개인 도구" > <label id="vector-user-links-dropdown-label" for="vector-user-links-dropdown-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button cdx-button--fake-button--enabled cdx-button--weight-quiet cdx-button--icon-only " aria-hidden="true" ><span class="vector-icon mw-ui-icon-ellipsis mw-ui-icon-wikimedia-ellipsis"></span> <span class="vector-dropdown-label-text">개인 도구</span> </label> <div class="vector-dropdown-content"> <div id="p-personal" class="vector-menu mw-portlet mw-portlet-personal user-links-collapsible-item" title="사용자 메뉴" > <div class="vector-menu-content"> <ul class="vector-menu-content-list"> <li id="pt-sitesupport" class="user-links-collapsible-item mw-list-item"><a href="//donate.wikimedia.org/wiki/Special:FundraiserRedirector?utm_source=donate&utm_medium=sidebar&utm_campaign=C13_ko.wikipedia.org&uselang=ko"><span>기부</span></a></li><li id="pt-createaccount" class="user-links-collapsible-item mw-list-item"><a href="/w/index.php?title=%ED%8A%B9%EC%88%98:%EA%B3%84%EC%A0%95%EB%A7%8C%EB%93%A4%EA%B8%B0&returnto=%ED%95%AD%EC%84%B1%EA%B3%84" title="계정을 만들고 로그인하는 것이 좋습니다. 하지만 필수는 아닙니다"><span class="vector-icon mw-ui-icon-userAdd mw-ui-icon-wikimedia-userAdd"></span> <span>계정 만들기</span></a></li><li id="pt-login" class="user-links-collapsible-item mw-list-item"><a href="/w/index.php?title=%ED%8A%B9%EC%88%98:%EB%A1%9C%EA%B7%B8%EC%9D%B8&returnto=%ED%95%AD%EC%84%B1%EA%B3%84" title="위키백과에 로그인하면 여러가지 편리한 기능을 사용할 수 있습니다. [o]" accesskey="o"><span class="vector-icon mw-ui-icon-logIn mw-ui-icon-wikimedia-logIn"></span> <span>로그인</span></a></li> </ul> </div> </div> <div id="p-user-menu-anon-editor" class="vector-menu mw-portlet mw-portlet-user-menu-anon-editor" > <div class="vector-menu-heading"> 로그아웃한 편집자를 위한 문서 <a href="/wiki/%EB%8F%84%EC%9B%80%EB%A7%90:%EC%86%8C%EA%B0%9C" aria-label="편집에 관해 더 알아보기"><span>더 알아보기</span></a> </div> <div class="vector-menu-content"> <ul class="vector-menu-content-list"> <li id="pt-anoncontribs" class="mw-list-item"><a href="/wiki/%ED%8A%B9%EC%88%98:%EB%82%B4%EA%B8%B0%EC%97%AC" title="이 IP 주소의 편집 목록 [y]" accesskey="y"><span>기여</span></a></li><li id="pt-anontalk" class="mw-list-item"><a href="/wiki/%ED%8A%B9%EC%88%98:%EB%82%B4%EC%82%AC%EC%9A%A9%EC%9E%90%ED%86%A0%EB%A1%A0" title="현재 사용하는 IP 주소에 대한 토론 문서 [n]" accesskey="n"><span>토론</span></a></li> </ul> </div> </div> </div> </div> </nav> </div> </header> </div> <div class="mw-page-container"> <div class="mw-page-container-inner"> <div class="vector-sitenotice-container"> <div id="siteNotice"></div> </div> <div class="vector-column-start"> <div class="vector-main-menu-container"> <div id="mw-navigation"> <nav id="mw-panel" class="vector-main-menu-landmark" aria-label="사이트"> <div id="vector-main-menu-pinned-container" class="vector-pinned-container"> </div> </nav> </div> </div> <div class="vector-sticky-pinned-container"> <nav id="mw-panel-toc" aria-label="목차" data-event-name="ui.sidebar-toc" class="mw-table-of-contents-container vector-toc-landmark"> <div id="vector-toc-pinned-container" class="vector-pinned-container"> <div id="vector-toc" class="vector-toc vector-pinnable-element"> <div class="vector-pinnable-header vector-toc-pinnable-header vector-pinnable-header-pinned" data-feature-name="toc-pinned" data-pinnable-element-id="vector-toc" > <h2 class="vector-pinnable-header-label">목차</h2> <button class="vector-pinnable-header-toggle-button vector-pinnable-header-pin-button" data-event-name="pinnable-header.vector-toc.pin">사이드바로 이동</button> <button class="vector-pinnable-header-toggle-button vector-pinnable-header-unpin-button" data-event-name="pinnable-header.vector-toc.unpin">숨기기</button> </div> <ul class="vector-toc-contents" id="mw-panel-toc-list"> <li id="toc-mw-content-text" class="vector-toc-list-item vector-toc-level-1"> <a href="#" class="vector-toc-link"> <div class="vector-toc-text">처음 위치</div> </a> </li> <li id="toc-쌍성계" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#쌍성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">1</span> <span>쌍성계</span> </div> </a> <ul id="toc-쌍성계-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-다중성계" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#다중성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">2</span> <span>다중성계</span> </div> </a> <ul id="toc-다중성계-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-계층_체계" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#계층_체계"> <div class="vector-toc-text"> <span class="vector-toc-numb">3</span> <span>계층 체계</span> </div> </a> <button aria-controls="toc-계층_체계-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> <span class="vector-icon mw-ui-icon-wikimedia-expand"></span> <span>계층 체계 하위섹션 토글하기</span> </button> <ul id="toc-계층_체계-sublist" class="vector-toc-list"> <li id="toc-삼중성계" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#삼중성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">3.1</span> <span>삼중성계</span> </div> </a> <ul id="toc-삼중성계-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-삼중성계_이상" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#삼중성계_이상"> <div class="vector-toc-text"> <span class="vector-toc-numb">3.2</span> <span>삼중성계 이상</span> </div> </a> <ul id="toc-삼중성계_이상-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-트라페지아" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#트라페지아"> <div class="vector-toc-text"> <span class="vector-toc-numb">3.3</span> <span>트라페지아</span> </div> </a> <ul id="toc-트라페지아-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-명칭_및_명명법" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#명칭_및_명명법"> <div class="vector-toc-text"> <span class="vector-toc-numb">4</span> <span>명칭 및 명명법</span> </div> </a> <button aria-controls="toc-명칭_및_명명법-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> <span class="vector-icon mw-ui-icon-wikimedia-expand"></span> <span>명칭 및 명명법 하위섹션 토글하기</span> </button> <ul id="toc-명칭_및_명명법-sublist" class="vector-toc-list"> <li id="toc-다중성계_명칭" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#다중성계_명칭"> <div class="vector-toc-text"> <span class="vector-toc-numb">4.1</span> <span>다중성계 명칭</span> </div> </a> <ul id="toc-다중성계_명칭-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-다중성성표에서의_명명법" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#다중성성표에서의_명명법"> <div class="vector-toc-text"> <span class="vector-toc-numb">4.2</span> <span>다중성성표에서의 명명법</span> </div> </a> <ul id="toc-다중성성표에서의_명명법-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-대표적인_예" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#대표적인_예"> <div class="vector-toc-text"> <span class="vector-toc-numb">5</span> <span>대표적인 예</span> </div> </a> <button aria-controls="toc-대표적인_예-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> <span class="vector-icon mw-ui-icon-wikimedia-expand"></span> <span>대표적인 예 하위섹션 토글하기</span> </button> <ul id="toc-대표적인_예-sublist" class="vector-toc-list"> <li id="toc-쌍성계_2" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#쌍성계_2"> <div class="vector-toc-text"> <span class="vector-toc-numb">5.1</span> <span>쌍성계</span> </div> </a> <ul id="toc-쌍성계_2-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-삼중성계_2" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#삼중성계_2"> <div class="vector-toc-text"> <span class="vector-toc-numb">5.2</span> <span>삼중성계</span> </div> </a> <ul id="toc-삼중성계_2-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-사중성계" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#사중성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">5.3</span> <span>사중성계</span> </div> </a> <ul id="toc-사중성계-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-오중성계" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#오중성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">5.4</span> <span>오중성계</span> </div> </a> <ul id="toc-오중성계-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-육중성계" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#육중성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">5.5</span> <span>육중성계</span> </div> </a> <ul id="toc-육중성계-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-칠중성계" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#칠중성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">6</span> <span>칠중성계</span> </div> </a> <ul id="toc-칠중성계-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-팔중성계" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#팔중성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">7</span> <span>팔중성계</span> </div> </a> <ul id="toc-팔중성계-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-구중성계" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#구중성계"> <div class="vector-toc-text"> <span class="vector-toc-numb">8</span> <span>구중성계</span> </div> </a> <ul id="toc-구중성계-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-각주" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#각주"> <div class="vector-toc-text"> <span class="vector-toc-numb">9</span> <span>각주</span> </div> </a> <ul id="toc-각주-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-외부_링크" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#외부_링크"> <div class="vector-toc-text"> <span class="vector-toc-numb">10</span> <span>외부 링크</span> </div> </a> <ul id="toc-외부_링크-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-같이_보기" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#같이_보기"> <div class="vector-toc-text"> <span class="vector-toc-numb">11</span> <span>같이 보기</span> </div> </a> <ul id="toc-같이_보기-sublist" class="vector-toc-list"> </ul> </li> </ul> </div> </div> </nav> </div> </div> <div class="mw-content-container"> <main id="content" class="mw-body"> <header class="mw-body-header vector-page-titlebar"> <nav aria-label="목차" class="vector-toc-landmark"> <div id="vector-page-titlebar-toc" class="vector-dropdown vector-page-titlebar-toc vector-button-flush-left" > <input type="checkbox" id="vector-page-titlebar-toc-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-vector-page-titlebar-toc" class="vector-dropdown-checkbox " aria-label="목차 토글" > <label id="vector-page-titlebar-toc-label" for="vector-page-titlebar-toc-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button cdx-button--fake-button--enabled cdx-button--weight-quiet cdx-button--icon-only " aria-hidden="true" ><span class="vector-icon mw-ui-icon-listBullet mw-ui-icon-wikimedia-listBullet"></span> <span class="vector-dropdown-label-text">목차 토글</span> </label> <div class="vector-dropdown-content"> <div id="vector-page-titlebar-toc-unpinned-container" class="vector-unpinned-container"> </div> </div> </div> </nav> <h1 id="firstHeading" class="firstHeading mw-first-heading"><span class="mw-page-title-main">항성계</span></h1> <div id="p-lang-btn" class="vector-dropdown mw-portlet mw-portlet-lang" > <input type="checkbox" id="p-lang-btn-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-p-lang-btn" class="vector-dropdown-checkbox mw-interlanguage-selector" aria-label="다른 언어로 문서를 방문합니다. 48개 언어로 읽을 수 있습니다" > <label id="p-lang-btn-label" for="p-lang-btn-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button cdx-button--fake-button--enabled cdx-button--weight-quiet cdx-button--action-progressive mw-portlet-lang-heading-48" aria-hidden="true" ><span class="vector-icon mw-ui-icon-language-progressive mw-ui-icon-wikimedia-language-progressive"></span> <span class="vector-dropdown-label-text">48개 언어</span> </label> <div class="vector-dropdown-content"> <div class="vector-menu-content"> <ul class="vector-menu-content-list"> <li class="interlanguage-link interwiki-af mw-list-item"><a href="https://af.wikipedia.org/wiki/Veelvoudige_ster" title="Veelvoudige ster – 아프리칸스어" lang="af" hreflang="af" data-title="Veelvoudige ster" data-language-autonym="Afrikaans" data-language-local-name="아프리칸스어" class="interlanguage-link-target"><span>Afrikaans</span></a></li><li class="interlanguage-link interwiki-ar mw-list-item"><a href="https://ar.wikipedia.org/wiki/%D9%86%D8%B8%D8%A7%D9%85_%D9%86%D8%AC%D9%85%D9%8A" title="نظام نجمي – 아랍어" lang="ar" hreflang="ar" data-title="نظام نجمي" data-language-autonym="العربية" data-language-local-name="아랍어" class="interlanguage-link-target"><span>العربية</span></a></li><li class="interlanguage-link interwiki-ast mw-list-item"><a href="https://ast.wikipedia.org/wiki/Sistema_estelar" title="Sistema estelar – 아스투리아어" lang="ast" hreflang="ast" data-title="Sistema estelar" data-language-autonym="Asturianu" data-language-local-name="아스투리아어" class="interlanguage-link-target"><span>Asturianu</span></a></li><li class="interlanguage-link interwiki-be mw-list-item"><a href="https://be.wikipedia.org/wiki/%D0%97%D0%BE%D1%80%D0%BD%D0%B0%D1%8F_%D1%81%D1%96%D1%81%D1%82%D1%8D%D0%BC%D0%B0" title="Зорная сістэма – 벨라루스어" lang="be" hreflang="be" data-title="Зорная сістэма" data-language-autonym="Беларуская" data-language-local-name="벨라루스어" class="interlanguage-link-target"><span>Беларуская</span></a></li><li class="interlanguage-link interwiki-be-x-old mw-list-item"><a href="https://be-tarask.wikipedia.org/wiki/%D0%97%D0%BE%D1%80%D0%BD%D0%B0%D1%8F_%D1%81%D1%8B%D1%81%D1%82%D1%8D%D0%BC%D0%B0" title="Зорная сыстэма – Belarusian (Taraškievica orthography)" lang="be-tarask" hreflang="be-tarask" data-title="Зорная сыстэма" data-language-autonym="Беларуская (тарашкевіца)" data-language-local-name="Belarusian (Taraškievica orthography)" class="interlanguage-link-target"><span>Беларуская (тарашкевіца)</span></a></li><li class="interlanguage-link interwiki-bg mw-list-item"><a href="https://bg.wikipedia.org/wiki/%D0%97%D0%B2%D0%B5%D0%B7%D0%B4%D0%BD%D0%B0_%D1%81%D0%B8%D1%81%D1%82%D0%B5%D0%BC%D0%B0" title="Звездна система – 불가리아어" lang="bg" hreflang="bg" data-title="Звездна система" data-language-autonym="Български" data-language-local-name="불가리아어" class="interlanguage-link-target"><span>Български</span></a></li><li class="interlanguage-link interwiki-ca mw-list-item"><a href="https://ca.wikipedia.org/wiki/Sistema_d%27estrelles" title="Sistema d'estrelles – 카탈로니아어" lang="ca" hreflang="ca" data-title="Sistema d'estrelles" data-language-autonym="Català" data-language-local-name="카탈로니아어" class="interlanguage-link-target"><span>Català</span></a></li><li class="interlanguage-link interwiki-en mw-list-item"><a href="https://en.wikipedia.org/wiki/Star_system" title="Star system – 영어" lang="en" hreflang="en" data-title="Star system" data-language-autonym="English" data-language-local-name="영어" class="interlanguage-link-target"><span>English</span></a></li><li class="interlanguage-link interwiki-es mw-list-item"><a href="https://es.wikipedia.org/wiki/Sistema_estelar" title="Sistema estelar – 스페인어" lang="es" hreflang="es" data-title="Sistema estelar" data-language-autonym="Español" data-language-local-name="스페인어" class="interlanguage-link-target"><span>Español</span></a></li><li class="interlanguage-link interwiki-et mw-list-item"><a href="https://et.wikipedia.org/wiki/T%C3%A4hes%C3%BCsteem" title="Tähesüsteem – 에스토니아어" lang="et" hreflang="et" data-title="Tähesüsteem" data-language-autonym="Eesti" data-language-local-name="에스토니아어" class="interlanguage-link-target"><span>Eesti</span></a></li><li class="interlanguage-link interwiki-eu mw-list-item"><a href="https://eu.wikipedia.org/wiki/Izar-sistema" title="Izar-sistema – 바스크어" lang="eu" hreflang="eu" data-title="Izar-sistema" data-language-autonym="Euskara" data-language-local-name="바스크어" class="interlanguage-link-target"><span>Euskara</span></a></li><li class="interlanguage-link interwiki-fa mw-list-item"><a href="https://fa.wikipedia.org/wiki/%D8%B3%D8%A7%D9%85%D8%A7%D9%86%D9%87_%D8%B3%D8%AA%D8%A7%D8%B1%D9%87%E2%80%8C%D8%A7%DB%8C" title="سامانه ستاره‌ای – 페르시아어" lang="fa" hreflang="fa" data-title="سامانه ستاره‌ای" data-language-autonym="فارسی" data-language-local-name="페르시아어" class="interlanguage-link-target"><span>فارسی</span></a></li><li class="interlanguage-link interwiki-fi mw-list-item"><a href="https://fi.wikipedia.org/wiki/T%C3%A4htij%C3%A4rjestelm%C3%A4" title="Tähtijärjestelmä – 핀란드어" lang="fi" hreflang="fi" data-title="Tähtijärjestelmä" data-language-autonym="Suomi" data-language-local-name="핀란드어" class="interlanguage-link-target"><span>Suomi</span></a></li><li class="interlanguage-link interwiki-fr mw-list-item"><a href="https://fr.wikipedia.org/wiki/Syst%C3%A8me_stellaire" title="Système stellaire – 프랑스어" lang="fr" hreflang="fr" data-title="Système stellaire" data-language-autonym="Français" data-language-local-name="프랑스어" class="interlanguage-link-target"><span>Français</span></a></li><li class="interlanguage-link interwiki-he mw-list-item"><a href="https://he.wikipedia.org/wiki/%D7%9E%D7%A2%D7%A8%D7%9B%D7%AA_%D7%9E%D7%A8%D7%95%D7%91%D7%AA_%D7%9B%D7%95%D7%9B%D7%91%D7%99%D7%9D" title="מערכת מרובת כוכבים – 히브리어" lang="he" hreflang="he" data-title="מערכת מרובת כוכבים" data-language-autonym="עברית" data-language-local-name="히브리어" class="interlanguage-link-target"><span>עברית</span></a></li><li class="interlanguage-link interwiki-hr mw-list-item"><a href="https://hr.wikipedia.org/wiki/Zvjezdani_sustav" title="Zvjezdani sustav – 크로아티아어" lang="hr" hreflang="hr" data-title="Zvjezdani sustav" data-language-autonym="Hrvatski" data-language-local-name="크로아티아어" class="interlanguage-link-target"><span>Hrvatski</span></a></li><li class="interlanguage-link interwiki-hu mw-list-item"><a href="https://hu.wikipedia.org/wiki/Csillagrendszer" title="Csillagrendszer – 헝가리어" lang="hu" hreflang="hu" data-title="Csillagrendszer" data-language-autonym="Magyar" data-language-local-name="헝가리어" class="interlanguage-link-target"><span>Magyar</span></a></li><li class="interlanguage-link interwiki-hy mw-list-item"><a href="https://hy.wikipedia.org/wiki/%D4%B1%D5%BD%D5%BF%D5%B2%D5%A1%D5%B5%D5%AB%D5%B6_%D5%B0%D5%A1%D5%B4%D5%A1%D5%AF%D5%A1%D6%80%D5%A3" title="Աստղային համակարգ – 아르메니아어" lang="hy" hreflang="hy" data-title="Աստղային համակարգ" data-language-autonym="Հայերեն" data-language-local-name="아르메니아어" class="interlanguage-link-target"><span>Հայերեն</span></a></li><li class="interlanguage-link interwiki-id mw-list-item"><a href="https://id.wikipedia.org/wiki/Sistem_bintang" title="Sistem bintang – 인도네시아어" lang="id" hreflang="id" data-title="Sistem bintang" data-language-autonym="Bahasa Indonesia" data-language-local-name="인도네시아어" class="interlanguage-link-target"><span>Bahasa Indonesia</span></a></li><li class="interlanguage-link interwiki-it mw-list-item"><a href="https://it.wikipedia.org/wiki/Sistema_stellare" title="Sistema stellare – 이탈리아어" lang="it" hreflang="it" data-title="Sistema stellare" data-language-autonym="Italiano" data-language-local-name="이탈리아어" class="interlanguage-link-target"><span>Italiano</span></a></li><li class="interlanguage-link interwiki-ja mw-list-item"><a href="https://ja.wikipedia.org/wiki/%E6%81%92%E6%98%9F%E7%B3%BB" title="恒星系 – 일본어" lang="ja" hreflang="ja" data-title="恒星系" data-language-autonym="日本語" data-language-local-name="일본어" class="interlanguage-link-target"><span>日本語</span></a></li><li class="interlanguage-link interwiki-jv mw-list-item"><a href="https://jv.wikipedia.org/wiki/Sistem_lintang" title="Sistem lintang – 자바어" lang="jv" hreflang="jv" data-title="Sistem lintang" data-language-autonym="Jawa" data-language-local-name="자바어" class="interlanguage-link-target"><span>Jawa</span></a></li><li class="interlanguage-link interwiki-kk mw-list-item"><a href="https://kk.wikipedia.org/wiki/%D0%96%D2%B1%D0%BB%D0%B4%D1%8B%D0%B7%D0%B4%D0%B0%D1%80_%D0%B6%D2%AF%D0%B9%D0%B5%D1%81%D1%96" title="Жұлдыздар жүйесі – 카자흐어" lang="kk" hreflang="kk" data-title="Жұлдыздар жүйесі" data-language-autonym="Қазақша" data-language-local-name="카자흐어" class="interlanguage-link-target"><span>Қазақша</span></a></li><li class="interlanguage-link interwiki-lb mw-list-item"><a href="https://lb.wikipedia.org/wiki/St%C3%A4resystem" title="Stäresystem – 룩셈부르크어" lang="lb" hreflang="lb" data-title="Stäresystem" data-language-autonym="Lëtzebuergesch" data-language-local-name="룩셈부르크어" class="interlanguage-link-target"><span>Lëtzebuergesch</span></a></li><li class="interlanguage-link interwiki-lt mw-list-item"><a href="https://lt.wikipedia.org/wiki/%C5%BDvaig%C5%BEd%C5%BEi%C5%B3_sistema" title="Žvaigždžių sistema – 리투아니아어" lang="lt" hreflang="lt" data-title="Žvaigždžių sistema" data-language-autonym="Lietuvių" data-language-local-name="리투아니아어" class="interlanguage-link-target"><span>Lietuvių</span></a></li><li class="interlanguage-link interwiki-lv mw-list-item"><a href="https://lv.wikipedia.org/wiki/Vair%C4%81kk%C4%81rt%C4%ABga_zvaig%C5%BE%C5%86u_sist%C4%93ma" title="Vairākkārtīga zvaigžņu sistēma – 라트비아어" lang="lv" hreflang="lv" data-title="Vairākkārtīga zvaigžņu sistēma" data-language-autonym="Latviešu" data-language-local-name="라트비아어" class="interlanguage-link-target"><span>Latviešu</span></a></li><li class="interlanguage-link interwiki-mk mw-list-item"><a href="https://mk.wikipedia.org/wiki/%D0%85%D0%B2%D0%B5%D0%B7%D0%B4%D0%B5%D0%BD_%D1%81%D0%B8%D1%81%D1%82%D0%B5%D0%BC" title="Ѕвезден систем – 마케도니아어" lang="mk" hreflang="mk" data-title="Ѕвезден систем" data-language-autonym="Македонски" data-language-local-name="마케도니아어" class="interlanguage-link-target"><span>Македонски</span></a></li><li class="interlanguage-link interwiki-ms mw-list-item"><a href="https://ms.wikipedia.org/wiki/Sistem_najam" title="Sistem najam – 말레이어" lang="ms" hreflang="ms" data-title="Sistem najam" data-language-autonym="Bahasa Melayu" data-language-local-name="말레이어" class="interlanguage-link-target"><span>Bahasa Melayu</span></a></li><li class="interlanguage-link interwiki-nl mw-list-item"><a href="https://nl.wikipedia.org/wiki/Stersysteem" title="Stersysteem – 네덜란드어" lang="nl" hreflang="nl" data-title="Stersysteem" data-language-autonym="Nederlands" data-language-local-name="네덜란드어" class="interlanguage-link-target"><span>Nederlands</span></a></li><li class="interlanguage-link interwiki-nn mw-list-item"><a href="https://nn.wikipedia.org/wiki/Multippel_stjerne" title="Multippel stjerne – 노르웨이어(니노르스크)" lang="nn" hreflang="nn" data-title="Multippel stjerne" data-language-autonym="Norsk nynorsk" data-language-local-name="노르웨이어(니노르스크)" class="interlanguage-link-target"><span>Norsk nynorsk</span></a></li><li class="interlanguage-link interwiki-no mw-list-item"><a href="https://no.wikipedia.org/wiki/Stjernesystem" title="Stjernesystem – 노르웨이어(보크말)" lang="nb" hreflang="nb" data-title="Stjernesystem" data-language-autonym="Norsk bokmål" data-language-local-name="노르웨이어(보크말)" class="interlanguage-link-target"><span>Norsk bokmål</span></a></li><li class="interlanguage-link interwiki-pnb mw-list-item"><a href="https://pnb.wikipedia.org/wiki/%D8%AA%D8%A7%D8%B1%DB%81_%D9%BE%D8%B1%D8%A8%D9%86%D8%AF%DA%BE" title="تارہ پربندھ – Western Punjabi" lang="pnb" hreflang="pnb" data-title="تارہ پربندھ" data-language-autonym="پنجابی" data-language-local-name="Western Punjabi" class="interlanguage-link-target"><span>پنجابی</span></a></li><li class="interlanguage-link interwiki-pt mw-list-item"><a href="https://pt.wikipedia.org/wiki/Sistema_estelar" title="Sistema estelar – 포르투갈어" lang="pt" hreflang="pt" data-title="Sistema estelar" data-language-autonym="Português" data-language-local-name="포르투갈어" class="interlanguage-link-target"><span>Português</span></a></li><li class="interlanguage-link interwiki-ro mw-list-item"><a href="https://ro.wikipedia.org/wiki/Sistem_stelar" title="Sistem stelar – 루마니아어" lang="ro" hreflang="ro" data-title="Sistem stelar" data-language-autonym="Română" data-language-local-name="루마니아어" class="interlanguage-link-target"><span>Română</span></a></li><li class="interlanguage-link interwiki-ru mw-list-item"><a href="https://ru.wikipedia.org/wiki/%D0%97%D0%B2%D1%91%D0%B7%D0%B4%D0%BD%D0%B0%D1%8F_%D1%81%D0%B8%D1%81%D1%82%D0%B5%D0%BC%D0%B0" title="Звёздная система – 러시아어" lang="ru" hreflang="ru" data-title="Звёздная система" data-language-autonym="Русский" data-language-local-name="러시아어" class="interlanguage-link-target"><span>Русский</span></a></li><li class="interlanguage-link interwiki-sco mw-list-item"><a href="https://sco.wikipedia.org/wiki/Starn_seestem" title="Starn seestem – 스코틀랜드어" lang="sco" hreflang="sco" data-title="Starn seestem" data-language-autonym="Scots" data-language-local-name="스코틀랜드어" class="interlanguage-link-target"><span>Scots</span></a></li><li class="interlanguage-link interwiki-sh mw-list-item"><a href="https://sh.wikipedia.org/wiki/Stelarni_sistem" title="Stelarni sistem – 세르비아-크로아티아어" lang="sh" hreflang="sh" data-title="Stelarni sistem" data-language-autonym="Srpskohrvatski / српскохрватски" data-language-local-name="세르비아-크로아티아어" class="interlanguage-link-target"><span>Srpskohrvatski / српскохрватски</span></a></li><li class="interlanguage-link interwiki-simple mw-list-item"><a href="https://simple.wikipedia.org/wiki/Star_system" title="Star system – Simple English" lang="en-simple" hreflang="en-simple" data-title="Star system" data-language-autonym="Simple English" data-language-local-name="Simple English" class="interlanguage-link-target"><span>Simple English</span></a></li><li class="interlanguage-link interwiki-sq mw-list-item"><a href="https://sq.wikipedia.org/wiki/Sistemi_yjor" title="Sistemi yjor – 알바니아어" lang="sq" hreflang="sq" data-title="Sistemi yjor" data-language-autonym="Shqip" data-language-local-name="알바니아어" class="interlanguage-link-target"><span>Shqip</span></a></li><li class="interlanguage-link interwiki-sr mw-list-item"><a href="https://sr.wikipedia.org/wiki/%D0%97%D0%B2%D0%B5%D0%B7%D0%B4%D0%B0%D0%BD%D0%B8_%D1%81%D0%B8%D1%81%D1%82%D0%B5%D0%BC" title="Звездани систем – 세르비아어" lang="sr" hreflang="sr" data-title="Звездани систем" data-language-autonym="Српски / srpski" data-language-local-name="세르비아어" class="interlanguage-link-target"><span>Српски / srpski</span></a></li><li class="interlanguage-link interwiki-sv mw-list-item"><a href="https://sv.wikipedia.org/wiki/Stj%C3%A4rnsystem" title="Stjärnsystem – 스웨덴어" lang="sv" hreflang="sv" data-title="Stjärnsystem" data-language-autonym="Svenska" data-language-local-name="스웨덴어" class="interlanguage-link-target"><span>Svenska</span></a></li><li class="interlanguage-link interwiki-th mw-list-item"><a href="https://th.wikipedia.org/wiki/%E0%B8%A3%E0%B8%B0%E0%B8%9A%E0%B8%9A%E0%B8%94%E0%B8%B2%E0%B8%A7%E0%B8%A4%E0%B8%81%E0%B8%A9%E0%B9%8C" title="ระบบดาวฤกษ์ – 태국어" lang="th" hreflang="th" data-title="ระบบดาวฤกษ์" data-language-autonym="ไทย" data-language-local-name="태국어" class="interlanguage-link-target"><span>ไทย</span></a></li><li class="interlanguage-link interwiki-tr mw-list-item"><a href="https://tr.wikipedia.org/wiki/Y%C4%B1ld%C4%B1z_sistemi" title="Yıldız sistemi – 터키어" lang="tr" hreflang="tr" data-title="Yıldız sistemi" data-language-autonym="Türkçe" data-language-local-name="터키어" class="interlanguage-link-target"><span>Türkçe</span></a></li><li class="interlanguage-link interwiki-uk mw-list-item"><a href="https://uk.wikipedia.org/wiki/%D0%97%D0%BE%D1%80%D1%8F%D0%BD%D0%B0_%D1%81%D0%B8%D1%81%D1%82%D0%B5%D0%BC%D0%B0" title="Зоряна система – 우크라이나어" lang="uk" hreflang="uk" data-title="Зоряна система" data-language-autonym="Українська" data-language-local-name="우크라이나어" class="interlanguage-link-target"><span>Українська</span></a></li><li class="interlanguage-link interwiki-uz mw-list-item"><a href="https://uz.wikipedia.org/wiki/Yulduz_tizimi" title="Yulduz tizimi – 우즈베크어" lang="uz" hreflang="uz" data-title="Yulduz tizimi" data-language-autonym="Oʻzbekcha / ўзбекча" data-language-local-name="우즈베크어" class="interlanguage-link-target"><span>Oʻzbekcha / ўзбекча</span></a></li><li class="interlanguage-link interwiki-vi mw-list-item"><a href="https://vi.wikipedia.org/wiki/H%E1%BB%87_sao" title="Hệ sao – 베트남어" lang="vi" hreflang="vi" data-title="Hệ sao" data-language-autonym="Tiếng Việt" data-language-local-name="베트남어" class="interlanguage-link-target"><span>Tiếng Việt</span></a></li><li class="interlanguage-link interwiki-wuu mw-list-item"><a href="https://wuu.wikipedia.org/wiki/%E6%81%92%E6%98%9F%E7%B3%BB%E7%BB%9F" title="恒星系统 – 우어" lang="wuu" hreflang="wuu" data-title="恒星系统" data-language-autonym="吴语" data-language-local-name="우어" class="interlanguage-link-target"><span>吴语</span></a></li><li class="interlanguage-link interwiki-zh mw-list-item"><a href="https://zh.wikipedia.org/wiki/%E6%81%86%E6%98%9F%E7%B3%BB%E7%B5%B1" title="恆星系統 – 중국어" lang="zh" hreflang="zh" data-title="恆星系統" data-language-autonym="中文" data-language-local-name="중국어" class="interlanguage-link-target"><span>中文</span></a></li> </ul> <div class="after-portlet after-portlet-lang"><span class="wb-langlinks-edit wb-langlinks-link"><a href="https://www.wikidata.org/wiki/Special:EntityPage/Q595871#sitelinks-wikipedia" title="언어 간 링크 편집" class="wbc-editpage">링크 편집</a></span></div> </div> </div> </div> </header> <div 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data-unpinned-container-id="vector-appearance-unpinned-container" > <div class="vector-pinnable-header-label">보이기</div> <button class="vector-pinnable-header-toggle-button vector-pinnable-header-pin-button" data-event-name="pinnable-header.vector-appearance.pin">사이드바로 이동</button> <button class="vector-pinnable-header-toggle-button vector-pinnable-header-unpin-button" data-event-name="pinnable-header.vector-appearance.unpin">숨기기</button> </div> </div> </div> </nav> </div> </div> <div id="bodyContent" class="vector-body" aria-labelledby="firstHeading" data-mw-ve-target-container> <div class="vector-body-before-content"> <div class="mw-indicators"> </div> <div id="siteSub" class="noprint">위키백과, 우리 모두의 백과사전.</div> </div> <div id="contentSub"><div id="mw-content-subtitle"></div></div> <div id="mw-content-text" class="mw-body-content"><div class="mw-content-ltr mw-parser-output" lang="ko" dir="ltr"><p><span class="nowrap"></span> </p> <div class="dablink hatnote"><span typeof="mw:File"><a href="/wiki/%EC%9C%84%ED%82%A4%EB%B0%B1%EA%B3%BC:%EB%8F%99%EC%9D%8C%EC%9D%B4%EC%9D%98%EC%96%B4_%EB%AC%B8%EC%84%9C" title="위키백과:동음이의어 문서"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Disambig_grey.svg/23px-Disambig_grey.svg.png" decoding="async" width="23" height="18" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Disambig_grey.svg/35px-Disambig_grey.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Disambig_grey.svg/46px-Disambig_grey.svg.png 2x" data-file-width="260" data-file-height="200" /></a></span> <b>삼중성</b>은 여기로 연결됩니다. 다른 뜻에 대해서는 <a href="/wiki/%EC%82%BC%EC%A4%91%EC%84%B1_(%EB%8F%99%EC%9D%8C%EC%9D%B4%EC%9D%98)" class="mw-disambig" title="삼중성 (동음이의)">삼중성 (동음이의)</a> 문서를 참고하십시오.</div> <p><b>항성계</b>(恒星系, <span style="font-size: smaller;"><a href="/wiki/%EC%98%81%EC%96%B4" title="영어">영어</a>: </span><span lang="en">star system 또는 stellar system</span>)는 서로의 <a href="/wiki/%EC%A4%91%EB%A0%A5" title="중력">중력</a>에 묶여서 <a href="/wiki/%EC%A7%88%EB%9F%89%EC%A4%91%EC%8B%AC" class="mw-redirect" title="질량중심">질량중심</a>을 기준으로 <a href="/wiki/%EA%B3%B5%EC%A0%84" title="공전">공전</a>을 하는 <a href="/wiki/%ED%95%AD%EC%84%B1" title="항성">항성</a>들을 일컫는 말이다. 다수의 항성들이 중력에 묶여 있는 상태는 보통 <a href="/wiki/%EC%84%B1%EB%8B%A8" title="성단">성단</a>(성단은 다시 <a href="/wiki/%EC%82%B0%EA%B0%9C%EC%84%B1%EB%8B%A8" title="산개성단">산개성단</a>과 <a href="/wiki/%EA%B5%AC%EC%83%81%EC%84%B1%EB%8B%A8" title="구상성단">구상성단</a>으로 나뉜다) 또는 <a href="/wiki/%EC%9D%80%ED%95%98" title="은하">은하계</a>라고 부르며, 넓게 보면 이들까지 항성계에 포함시킬 수 있다. <a href="/wiki/%EB%8B%A8%EB%8F%85%EC%84%B1" class="mw-redirect" title="단독성">단독성</a> 주위를 공전하는 <a href="/wiki/%ED%96%89%EC%84%B1%EA%B3%84" title="행성계">행성계</a>를 포함하여 일컫기도 한다. </p> <meta property="mw:PageProp/toc" /> <div class="mw-heading mw-heading2"><h2 id="쌍성계"><span id=".EC.8C.8D.EC.84.B1.EA.B3.84"></span>쌍성계</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=1" title="부분 편집: 쌍성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <style data-mw-deduplicate="TemplateStyles:r34311305">.mw-parser-output .hatnote{}.mw-parser-output div.hatnote{padding-left:1.6em;margin-bottom:0.5em}.mw-parser-output .hatnote i{font-style:normal}.mw-parser-output .hatnote+link+.hatnote{margin-top:-0.5em}</style><div role="note" class="hatnote navigation-not-searchable"><span typeof="mw:File"><span><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/Icons8_flat_search.svg/18px-Icons8_flat_search.svg.png" decoding="async" width="18" height="18" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/Icons8_flat_search.svg/27px-Icons8_flat_search.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/52/Icons8_flat_search.svg/36px-Icons8_flat_search.svg.png 2x" data-file-width="512" data-file-height="512" /></span></span> 이 부분의 본문은 <a href="/wiki/%EC%8C%8D%EC%84%B1" title="쌍성">쌍성</a>입니다.</div> <figure typeof="mw:File/Thumb"><a href="/wiki/%ED%8C%8C%EC%9D%BC:Sirius_A_and_B_Hubble_photo.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f3/Sirius_A_and_B_Hubble_photo.jpg/150px-Sirius_A_and_B_Hubble_photo.jpg" decoding="async" width="150" height="164" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f3/Sirius_A_and_B_Hubble_photo.jpg/225px-Sirius_A_and_B_Hubble_photo.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f3/Sirius_A_and_B_Hubble_photo.jpg/300px-Sirius_A_and_B_Hubble_photo.jpg 2x" data-file-width="369" data-file-height="403" /></a><figcaption>시리우스는 쌍성으로 <a href="/wiki/%EC%A3%BC%EA%B3%84%EC%97%B4" title="주계열">주계열성</a> A와 <a href="/wiki/%EB%B0%B1%EC%83%89%EC%99%9C%EC%84%B1" title="백색왜성">백색왜성</a> B로 이루어져 있다.</figcaption></figure> <p>2개의 항성으로 구성된 항성계를 <b><a href="/wiki/%EC%8C%8D%EC%84%B1" title="쌍성">쌍성계</a></b>(binary star system, 雙星系)라고 한다. <a href="/wiki/%EA%B8%B0%EC%A1%B0%EB%A0%A5" class="mw-redirect" title="기조력">기조력</a>이나 다른 <a href="/wiki/%EC%B2%9C%EC%B2%B4" title="천체">천체</a>로부터의 중력간섭, 항성간 질량 교환이 없을 경우 쌍성계는 안정되게 존속하며, 두 별은 <a href="/wiki/%EC%A7%88%EB%9F%89%EC%A4%91%EC%8B%AC" class="mw-redirect" title="질량중심">질량중심</a>을 기준으로 <a href="/wiki/%ED%83%80%EC%9B%90" title="타원">타원</a>형의 궤도를 따라 공전한다. (<a href="/wiki/%EC%9D%B4%EC%B2%B4%EB%AC%B8%EC%A0%9C" class="mw-redirect" title="이체문제">이체문제</a> 참조) </p><p>쌍성계의 예로 <a href="/wiki/%EC%8B%9C%EB%A6%AC%EC%9A%B0%EC%8A%A4" title="시리우스">시리우스</a>, <a href="/wiki/%ED%94%84%EB%A1%9C%ED%82%A4%EC%98%A8" title="프로키온">프로키온</a>, <a href="/wiki/%EB%B0%B1%EC%A1%B0%EC%9E%90%EB%A6%AC_X-1" title="백조자리 X-1">백조자리 X-1</a>, <a href="/wiki/%EC%95%8C%ED%8C%8C_%EC%84%BC%ED%83%80%EC%9A%B0%EB%A6%AC" class="mw-redirect" title="알파 센타우리">알파 센타우리</a>(<a href="/wiki/%ED%94%84%EB%A1%9D%EC%8B%9C%EB%A7%88_%EC%84%BC%ED%83%80%EC%9A%B0%EB%A6%AC" class="mw-redirect" title="프록시마 센타우리">프록시마 센타우리</a> 제외) 등이 있다. 이 중 백조자리 X-1은 둘 중 하나가 <a href="/wiki/%EB%B8%94%EB%9E%99%ED%99%80" title="블랙홀">블랙홀</a>로 추측된다. </p> <div class="mw-heading mw-heading2"><h2 id="다중성계"><span id=".EB.8B.A4.EC.A4.91.EC.84.B1.EA.B3.84"></span>다중성계</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=2" title="부분 편집: 다중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure typeof="mw:File/Thumb"><a href="/wiki/%ED%8C%8C%EC%9D%BC:HD188753_orbit.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/7/7c/HD188753_orbit.jpg/150px-HD188753_orbit.jpg" decoding="async" width="150" height="120" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/7c/HD188753_orbit.jpg/225px-HD188753_orbit.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/7c/HD188753_orbit.jpg/300px-HD188753_orbit.jpg 2x" data-file-width="800" data-file-height="640" /></a><figcaption>삼중성계 <a href="/wiki/HD_188753" title="HD 188753">HD 188753</a>의 상상도.</figcaption></figure> <p>세 개 이상의 항성이 <a href="/wiki/%EC%A4%91%EB%A0%A5" title="중력">중력</a>으로 묶여 있는 항성계를 <b>다중성계</b>(multiple star system, 多重星系)라고 한다. 이보다 넓은 개념으로 <b>다중성</b>(多重星)이 있는데 이는 지구에서 보았을 때 세 개 이상의 별로 보이는 <a href="/wiki/%EC%B2%9C%EC%B2%B4" title="천체">천체</a>들을 일컫는 말이다. 다중성은 실제 중력에 의해 묶여 있을 수도 있고 단순히 지구에서 보았을 때 같은 방향에 있어서 가까이 있는 것처럼 보이는 안시다중성일 수도 있다. </p><p>다중성계 중 다수를 차지하는 것은 세 개의 별로 이루어진 삼중성계이다. 네 개로 이루어졌을 경우 사중성계, 다섯 개로 이루어졌을 경우 오중성계 등으로 부른다. </p><p>삼중성계에서 세 개의 별은 각자의 <a href="/wiki/%EC%A7%88%EB%9F%89_%EC%A4%91%EC%8B%AC" title="질량 중심">질량 중심</a>을 공전한다. 보통 삼중성계는 두 별이 매우 가까이 붙어 있으면서 나머지 별을 멀리서 공전하는 계층 구조를 형성하고 있다. 삼중성계 뿐 아니라 더 많은 별들로 이루어진 다른 다수의 다중성계들도 계층 구조를 형성하고 있다. </p> <div class="mw-heading mw-heading2"><h2 id="계층_체계"><span id=".EA.B3.84.EC.B8.B5_.EC.B2.B4.EA.B3.84"></span>계층 체계</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=3" title="부분 편집: 계층 체계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure typeof="mw:File/Thumb"><a href="/wiki/%ED%8C%8C%EC%9D%BC:Smoke_ring_for_a_halo.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/9f/Smoke_ring_for_a_halo.jpg/150px-Smoke_ring_for_a_halo.jpg" decoding="async" width="150" height="198" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/9f/Smoke_ring_for_a_halo.jpg/225px-Smoke_ring_for_a_halo.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/9f/Smoke_ring_for_a_halo.jpg/300px-Smoke_ring_for_a_halo.jpg 2x" data-file-width="1280" data-file-height="1690" /></a><figcaption><a href="/wiki/%EC%B9%B4%EB%A9%9C%EB%A0%88%EC%98%A8%EC%9E%90%EB%A6%AC_DI" title="카멜레온자리 DI">카멜레온자리 DI</a>. 우리 눈에는 두 개의 별로 이루어진 것처럼 보이나 사실 두 별은 각각 쌍성으로 DI는 사중성계가 된다.<sup id="cite_ref-1" class="reference"><a href="#cite_note-1"><span class="cite-bracket">[</span>1<span class="cite-bracket">]</span></a></sup></figcaption></figure> <p>다중성계 대부분은 이른바 '계층 체계'(hierarchical system)를 이루고 있다. 이는 어떤 계(系)에 속한 구성원들은 각자가 더 작은 하위 계를 이루고 있으며 이들 작은 계 자체가 하나의 천체처럼 작용하여 상대방 하위 계와 서로의 <a href="/wiki/%EC%A7%88%EB%9F%89_%EC%A4%91%EC%8B%AC" title="질량 중심">질량 중심</a>을 공전한다는 뜻이다. 하위 계는 다시 차하위 계로 나눠질 수 있으며 마찬가지로 차하위 계의 구성원들이 뭉쳐서 하위 계의 단독 천체처럼 작동한다.<sup id="cite_ref-2" class="reference"><a href="#cite_note-2"><span class="cite-bracket">[</span>2<span class="cite-bracket">]</span></a></sup> 같은 계층 수준에서는 가까이 붙어 있는 <a href="/wiki/%EC%8C%8D%EC%84%B1" title="쌍성">쌍성</a>들을 홑별처럼 취급하여 <a href="/wiki/%EC%9D%B4%EC%B2%B4_%EB%AC%B8%EC%A0%9C" title="이체 문제">이체 문제</a>로 설명할 수 있다. 불안정한 트라페지아(trapezia) 계나 <a href="/wiki/%EC%84%B1%EB%8B%A8" title="성단">성단</a>과 <a href="/wiki/%EC%9D%80%ED%95%98" title="은하">은하</a> 내 다수의 항성들이 보여주는 보다 복잡한 <a href="/wiki/%EB%8F%99%EC%97%AD%ED%95%99" title="동역학">동역학</a>과는 달리, 계층 체계에서는 상위 공전궤도와 하위 공전궤도 사이에 상호작용이 거의 일어나지 않는다. 따라서 항성들의 움직임은 계의 질량 중심을 두고 대체로 안정적인<sup id="cite_ref-toko_3-0" class="reference"><a href="#cite_note-toko-3"><span class="cite-bracket">[</span>3<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-heintz1_4-0" class="reference"><a href="#cite_note-heintz1-4"><span class="cite-bracket">[</span>4<span class="cite-bracket">]</span></a></sup> 케플러 궤도를 유지하게 된다.<sup id="cite_ref-5" class="reference"><a href="#cite_note-5"><span class="cite-bracket">[</span>5<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading3"><h3 id="삼중성계"><span id=".EC.82.BC.EC.A4.91.EC.84.B1.EA.B3.84"></span>삼중성계</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=4" title="부분 편집: 삼중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <p>'물리적' 삼중성계에서 각각의 별은 <a href="/wiki/%EC%A4%91%EB%A0%A5" title="중력">중력</a>으로 묶여 계의 질량 중심을 돈다. 보통 삼중성계 중 두 별은 가까이에서 쌍성을 구성하며 세 번째 별은 쌍성계 구성원의 궤도보다 훨씬 큰 궤도를 그리면서 쌍성계를 돈다. 이 배열을 '계층'(hierarchical)이라고 부른다.<sup id="cite_ref-6" class="reference"><a href="#cite_note-6"><span class="cite-bracket">[</span>6<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-evans_7-0" class="reference"><a href="#cite_note-evans-7"><span class="cite-bracket">[</span>7<span class="cite-bracket">]</span></a></sup> 만약 쌍성계 궤도와 세 번째 별의 궤도 크기가 편차가 크지 않다면 계는 동역학적으로 불안정해져서 별 하나가 계에서 이탈할 것이다.<sup id="cite_ref-8" class="reference"><a href="#cite_note-8"><span class="cite-bracket">[</span>8<span class="cite-bracket">]</span></a></sup> 그러나 우리 눈으로 볼 때 삼중성처럼 보이는 모든 천체들이 실제로 중력으로 묶여 있는 것은 아니며 보통 세 번째 천체가 쌍성과 물리적으로 묶이지 않은 경우도 있는데 대표적인 예가 <a href="/w/index.php?title=%EC%84%B8%ED%8E%98%EC%9A%B0%EC%8A%A4%EC%9E%90%EB%A6%AC_%EB%B2%A0%ED%83%80&action=edit&redlink=1" class="new" title="세페우스자리 베타 (없는 문서)">세페우스자리 베타</a>이다. 혹은 드물지만 구성원 셋이 사실상 중력으로 묶이지 않은 안시 삼중성인 경우도 있으며 <a href="/wiki/%EB%B1%80%EC%9E%90%EB%A6%AC_%EA%B0%90%EB%A7%88" title="뱀자리 감마">뱀자리 감마</a>가 그 좋은 예이다. </p> <div class="mw-heading mw-heading3"><h3 id="삼중성계_이상"><span id=".EC.82.BC.EC.A4.91.EC.84.B1.EA.B3.84_.EC.9D.B4.EC.83.81"></span>삼중성계 이상</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=5" title="부분 편집: 삼중성계 이상"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/%ED%8C%8C%EC%9D%BC:Mobile-diagrams.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/c/c1/Mobile-diagrams.png/220px-Mobile-diagrams.png" decoding="async" width="220" height="263" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/c/c1/Mobile-diagrams.png 1.5x" data-file-width="300" data-file-height="359" /></a><figcaption> 모빌 도표: <div><ol style="list-style-type:lower-alpha"><li style="margin-left:-12px;">다중</li><li style="margin-left:-12px;">단순, 쌍성계</li><li style="margin-left:-12px;">단순, 삼중성계, 2계층</li><li style="margin-left:-12px;">단순, 사중성계, 2계층</li><li style="margin-left:-12px;">단순, 사중성계, 3계층</li><li style="margin-left:-12px;">단순, 오중성계, 4계층</li></ol></div></figcaption></figure> <p>별 세 개 이상으로 구성된 항성계는 여러 종류의 복잡한 배열을 가질 수 있는데 1968년 에반스는 이를 '<a href="/wiki/%EB%AA%A8%EB%B9%8C" title="모빌">모빌</a> 도표'(mobile diagram)로 명명, 소개했다. '모빌' 이름이 붙은 이유는 에반스의 그림이 천장으로부터 아래로 늘어뜨린 모빌과 비슷하게 생겼기 때문이다. 오른쪽 그림에 예시가 나와 있다. <a href="/wiki/%EB%85%B8%EB%93%9C" class="mw-disambig" title="노드">노드</a>에서 나오는 가지 수는 상위 계가 하위 계로 분해될 수 있는 개수를 뜻한다. 이 그림에서 노드 1개에 자식이 둘 이상 딸려 있을 경우, 즉 어떤 하위 계가 크기가 크게 차이나지 않는 공전궤도 두 개 이상으로 이루어졌을 경우를 '다중'(multiplex) 구조로 부른다. 앞서 설명한 삼중성계 예처럼 다중형태 계는 불안정하기 때문에 보통 다중성은 '단순'(simplex) 구조로 이루어졌을 확률이 높다. 단순 구조란 각각의 단계에서 자식이 정확히 둘만 있는 것을 뜻한다. 단계의 개수를 '계층'(hierarchy)이라고 한다.<sup id="cite_ref-9" class="reference"><a href="#cite_note-9"><span class="cite-bracket">[</span>9<span class="cite-bracket">]</span></a></sup> </p> <ul><li>(a)는 단일 계층에 하위 계가 없는 다중 구조이다.</li></ul> <ul><li>(b)는 전형적인 쌍성계로 단일 계층이다.</li> <li>단순+2계층 항성계의 경우 (c)처럼 구성원이 셋이거나(삼중성계), (d)처럼 구성원이 넷일 수 있다.(사중성계)</li> <li>단순+3계층 항성계의 경우 구성원은 최소 넷부터 최대 여덟까지 가능하다. (e)는 3계층 사중성계로 쌍성계를 구성원 하나가 멀리 떨어져 돌고 있는데, 이 쌍성계의 구성원 둘 중 하나는 다시 더 가까이 붙어 돌고 있는 쌍성이다.</li> <li>3계층 항성계 중 대표적인 것은 <a href="/wiki/%EC%B9%B4%EC%8A%A4%ED%86%A0%EB%A5%B4_(%ED%95%AD%EC%84%B1)" title="카스토르 (항성)">카스토르</a>이다. 이 별은 우리 눈에는 <a href="/wiki/%EC%95%88%EC%8B%9C%EC%8C%8D%EC%84%B1" class="mw-redirect" title="안시쌍성">안시쌍성</a>처럼 보이나 구성원 둘은 각자가 <a href="/wiki/%EB%B6%84%EA%B4%91%EC%8C%8D%EC%84%B1" class="mw-redirect" title="분광쌍성">분광쌍성</a>이다. 여기까지는 (d)와 같은 2계층 사중성계로 보인다. 그러나 이 사중성계 주위를 어두운 구성원이 멀리 떨어져 돌고 있으며 이 구성원은 <a href="/wiki/%EC%A0%81%EC%83%89%EC%99%9C%EC%84%B1" title="적색왜성">적색왜성</a> 두 개로 이루어진 쌍성이다. 따라서 카스토르는 3계층의 육중성계가 된다.<sup id="cite_ref-10" class="reference"><a href="#cite_note-10"><span class="cite-bracket">[</span>10<span class="cite-bracket">]</span></a></sup></li> <li>A. A. 토코비닌의 1999년 기준 다중성성표에 등장하는 최대 계층 수는 4이다.<sup id="cite_ref-11" class="reference"><a href="#cite_note-11"><span class="cite-bracket">[</span>11<span class="cite-bracket">]</span></a></sup> 예를 들면 <a href="/w/index.php?title=%EA%B8%80%EB%A6%AC%EC%A0%9C_644&action=edit&redlink=1" class="new" title="글리제 644 (없는 문서)">글리제 644A</a>와 644B는 가까이 붙어 있는 안시이중성처럼 보이지만 B가 분광쌍성이기 때문에 실제로는 삼중성계이다. 이 삼중성계를 멀리 떨어져 있는 글리제 643과 더 멀리 떨어져 있는 글리제 644C가 돌고 있는데 이들은 글리제 644AB와 <a href="/wiki/%EA%B3%A0%EC%9C%A0%EC%9A%B4%EB%8F%99" title="고유운동">고유운동</a>을 함께 하므로 중력적으로 묶여 있는 것으로 보인다. 가정이 맞다면 이 계는 (f)와 같은 4계층의 오중성계가 된다.<sup id="cite_ref-12" class="reference"><a href="#cite_note-12"><span class="cite-bracket">[</span>12<span class="cite-bracket">]</span></a></sup></li></ul> <p>앞서 설명한 사례보다 더 높은 계층도 존재할 수 있다.<sup id="cite_ref-evans_7-1" class="reference"><a href="#cite_note-evans-7"><span class="cite-bracket">[</span>7<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-13" class="reference"><a href="#cite_note-13"><span class="cite-bracket">[</span>13<span class="cite-bracket">]</span></a></sup> 이렇게 복잡한 계층을 지니는 항성계는 안정적이거나 혹은 계 내부의 <a href="/wiki/%EC%84%AD%EB%8F%99_(%EC%B2%9C%EB%AC%B8%ED%95%99)" title="섭동 (천문학)">섭동</a>으로 불안정할 수 있다.<sup id="cite_ref-14" class="reference"><a href="#cite_note-14"><span class="cite-bracket">[</span>14<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-15" class="reference"><a href="#cite_note-15"><span class="cite-bracket">[</span>15<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-16" class="reference"><a href="#cite_note-16"><span class="cite-bracket">[</span>16<span class="cite-bracket">]</span></a></sup> 복잡한 다중성계가 시간이 지나면서 삼중성계나 사중성계처럼 덜 복잡한 형태로 분해된다는 주장도 있다.<sup id="cite_ref-17" class="reference"><a href="#cite_note-17"><span class="cite-bracket">[</span>17<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-18" class="reference"><a href="#cite_note-18"><span class="cite-bracket">[</span>18<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading3"><h3 id="트라페지아"><span id=".ED.8A.B8.EB.9D.BC.ED.8E.98.EC.A7.80.EC.95.84"></span>트라페지아</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=6" title="부분 편집: 트라페지아"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <p>트라페지아는 일반적으로 매우 젊고 불안정한 계이다. 이 계는 항성 요람 영역(stellar nurseries)에서 생겨나는 것으로 보이며 안정적인 다중성계로 빠르게 쪼개진다. 트라페지아가 쪼개지는 과정에서 구성원이 튕겨져 나갈 수 있는데 이런 별을 폭주성으로 부른다.<sup id="cite_ref-heintztrapezia_19-0" class="reference"><a href="#cite_note-heintztrapezia-19"><span class="cite-bracket">[</span>19<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-20" class="reference"><a href="#cite_note-20"><span class="cite-bracket">[</span>20<span class="cite-bracket">]</span></a></sup> 트라페지아라는 명칭은 <a href="/wiki/%EC%98%A4%EB%A6%AC%EC%98%A8_%EC%84%B1%EC%9A%B4" title="오리온 성운">오리온 성운</a> 중심부에 있는 다중성계인 <a href="/wiki/%EC%82%AC%EB%8B%A4%EB%A6%AC%EA%BC%B4%EC%84%B1%EB%8B%A8" title="사다리꼴성단">사다리꼴성단</a>의 이름을 따 온 것이다.<sup id="cite_ref-heintztrapezia_19-1" class="reference"><a href="#cite_note-heintztrapezia-19"><span class="cite-bracket">[</span>19<span class="cite-bracket">]</span></a></sup> 트라페지아 계는 흔하게 존재하며 보통 밝은 <a href="/wiki/%EC%84%B1%EC%9A%B4" title="성운">성운</a> 근처나 내부에 있다. 계 구성원 사이에 정해진 계층 구조는 없으며 질량중심 또한 특정지점에 고정되어 있지 않다. 대신 구성원들은 위치를 동시에 바꿔서 질량중심의 위치를 옮기는 방식으로 안정된 궤도를 유지하려 하는데 이 관계를 '상호작용'(interplay)이라고 한다.<sup id="cite_ref-Heintz_1978_68_21-0" class="reference"><a href="#cite_note-Heintz_1978_68-21"><span class="cite-bracket">[</span>21<span class="cite-bracket">]</span></a></sup> 이런 별들은 종국적으로 가까이 붙어 있는 쌍성계와 이들을 멀리 떨어져 도는 짝별 구조로 안정화되며 구성원 중 일부는 빠른 속도로 우주공간에 내쳐지기도 한다.<sup id="cite_ref-Heintz_1978_68_21-1" class="reference"><a href="#cite_note-Heintz_1978_68-21"><span class="cite-bracket">[</span>21<span class="cite-bracket">]</span></a></sup> 이런 과정은 쌍성계 둘 또는 다중성계끼리 충돌하는 과정에서 계를 탈출하는 폭주성을 설명해 주는데 대표적 예로 초당 200 km 속도로 움직이는 <a href="/wiki/%EB%A7%88%EC%B0%A8%EB%B6%80%EC%9E%90%EB%A6%AC_AE" title="마차부자리 AE">마차부자리 AE</a>, <a href="/wiki/%EB%B9%84%EB%91%98%EA%B8%B0%EC%9E%90%EB%A6%AC_%EB%AE%A4" title="비둘기자리 뮤">비둘기자리 뮤</a>, <a href="/wiki/%EC%96%91%EC%9E%90%EB%A6%AC_53" title="양자리 53">양자리 53</a>을 들 수 있다. 이들은 수백만 년 전 오리온 성운 내 사다리꼴성단에서 탈출한 것으로 추측된다.<sup id="cite_ref-Hoogerwerf_22-0" class="reference"><a href="#cite_note-Hoogerwerf-22"><span class="cite-bracket">[</span>22<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading2"><h2 id="명칭_및_명명법"><span id=".EB.AA.85.EC.B9.AD_.EB.B0.8F_.EB.AA.85.EB.AA.85.EB.B2.95"></span>명칭 및 명명법</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=7" title="부분 편집: 명칭 및 명명법"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <div class="mw-heading mw-heading3"><h3 id="다중성계_명칭"><span id=".EB.8B.A4.EC.A4.91.EC.84.B1.EA.B3.84_.EB.AA.85.EC.B9.AD"></span>다중성계 명칭</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=8" title="부분 편집: 다중성계 명칭"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <p>다중성계의 구성원들은 계의 명칭 뒤에 A, B, C...처럼 <a href="/wiki/%EB%A1%9C%EB%A7%88%EC%9E%90" title="로마자">로마자</a> <a href="/wiki/%EB%8C%80%EC%86%8C%EB%AC%B8%EC%9E%90" title="대소문자">대문자</a>를 붙여 구별한다. A와 B 두 구성원으로 이루어진 항성계는 AB로 표기한다. 대문자의 순서는 주성 A로부터 떨어져 있는 순서대로 B, C...를 붙인다.<sup id="cite_ref-Heintz19_23-0" class="reference"><a href="#cite_note-Heintz19-23"><span class="cite-bracket">[</span>23<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-fmt_24-0" class="reference"><a href="#cite_note-fmt-24"><span class="cite-bracket">[</span>24<span class="cite-bracket">]</span></a></sup> 기존의 별 근처에서 새로운 구성원이 발견될 경우 Aa, Ba처럼 로마자 소문자를 대문자 뒤에 붙여 구별한다.<sup id="cite_ref-fmt_24-1" class="reference"><a href="#cite_note-fmt-24"><span class="cite-bracket">[</span>24<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading3"><h3 id="다중성성표에서의_명명법"><span id=".EB.8B.A4.EC.A4.91.EC.84.B1.EC.84.B1.ED.91.9C.EC.97.90.EC.84.9C.EC.9D.98_.EB.AA.85.EB.AA.85.EB.B2.95"></span>다중성성표에서의 명명법</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=9" title="부분 편집: 다중성성표에서의 명명법"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/%ED%8C%8C%EC%9D%BC:Tokovinin-multiple-star-notation.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/8/83/Tokovinin-multiple-star-notation.png" decoding="async" width="177" height="240" class="mw-file-element" data-file-width="177" data-file-height="240" /></a><figcaption>토코비닌의 다중성성표는 계(系)를 아라비아 숫자로 표기하고 있다.</figcaption></figure> <p>A. A. 토코비닌의 다중성성표에서는 모빌도표상 구성원을 표기하는 기호로 로마자가 아닌 <a href="/wiki/%EC%95%84%EB%9D%BC%EB%B9%84%EC%95%84_%EC%88%AB%EC%9E%90" title="아라비아 숫자">아라비아 숫자</a>를 사용한다. 예를 들어 상기문단 모빌도표 그림 (d)의 경우 항성계 전체에는 숫자 1이 부여되며 주인별이 속한 하위 계에는 11, 짝별이 속한 하위 계에는 12가 부여된다. 이보다 더 아래의 차하위 계로 갈수록 부여되는 숫자의 수는 세 개, 네 개, 다섯 개로 늘어난다. 반면 중력으로 연결되지 않은 안시다중성의 경우 같은 숫자가 두 번 이상 사용된다. 예를 들어 서로 중력으로 묶이지 않은 A, B, C 세 구성원의 경우 AB와 AC에는 둘 다 같은 숫자 1이 부여될 것이다. 여기에서 B와 C가 각각 <a href="/wiki/%EC%8C%8D%EC%84%B1" title="쌍성">쌍성</a>으로 구성되어 있을 경우에는 각각 숫자 12와 13이 부여될 것이다.<sup id="cite_ref-25" class="reference"><a href="#cite_note-25"><span class="cite-bracket">[</span>25<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading2"><h2 id="대표적인_예"><span id=".EB.8C.80.ED.91.9C.EC.A0.81.EC.9D.B8_.EC.98.88"></span>대표적인 예</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=10" title="부분 편집: 대표적인 예"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <div class="mw-heading mw-heading3"><h3 id="쌍성계_2"><span id=".EC.8C.8D.EC.84.B1.EA.B3.84_2"></span>쌍성계</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=11" title="부분 편집: 쌍성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <ul><li><a href="/wiki/%EC%8B%9C%EB%A6%AC%EC%9A%B0%EC%8A%A4" title="시리우스">시리우스</a>. A형 <a href="/wiki/%EC%A3%BC%EA%B3%84%EC%97%B4%EC%84%B1" class="mw-redirect" title="주계열성">주계열성</a>과 <a href="/wiki/%EB%B0%B1%EC%83%89%EC%99%9C%EC%84%B1" title="백색왜성">백색왜성</a>으로 이뤄진 쌍성계이다.</li> <li><a href="/wiki/%ED%94%84%EB%A1%9C%ED%82%A4%EC%98%A8" title="프로키온">프로키온</a>. 시리우스와 같은 구조이다.</li> <li><a href="/wiki/%EB%AF%B8%EB%9D%BC_(%ED%95%AD%EC%84%B1)" title="미라 (항성)">미라</a>. <a href="/wiki/%EC%A0%81%EC%83%89%EA%B1%B0%EC%84%B1" title="적색거성">적색거성</a>과 백색왜성으로 이뤄졌다.</li> <li><a href="/wiki/%EB%A7%88%EC%B0%A8%EB%B6%80%EC%9E%90%EB%A6%AC_%EC%97%A1%EC%8B%A4%EB%A1%A0" title="마차부자리 엡실론">마차부자리 엡실론</a>. 식쌍성이다.</li> <li><a href="/wiki/%EC%8A%A4%ED%94%BC%EC%B9%B4" title="스피카">스피카</a></li> <li><a href="/wiki/%EC%B2%98%EB%85%80%EC%9E%90%EB%A6%AC_HW" title="처녀자리 HW">처녀자리 HW</a>. A 가 <a href="/wiki/%EC%A4%80%EC%99%9C%EC%84%B1" title="준왜성">준왜성</a>, B가 <a href="/wiki/%EC%A0%81%EC%83%89%EC%99%9C%EC%84%B1" title="적색왜성">적색왜성</a>이다</li></ul> <div class="mw-heading mw-heading3"><h3 id="삼중성계_2"><span id=".EC.82.BC.EC.A4.91.EC.84.B1.EA.B3.84_2"></span>삼중성계</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=12" title="부분 편집: 삼중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <ul><li><a href="/wiki/%EC%84%BC%ED%83%80%EC%9A%B0%EB%A3%A8%EC%8A%A4%EC%9E%90%EB%A6%AC_%EC%95%8C%ED%8C%8C" title="센타우루스자리 알파">센타우루스자리 알파</a>. A와 B로 이루어진 쌍성계를, <a href="/wiki/%EC%A0%81%EC%83%89%EC%99%9C%EC%84%B1" title="적색왜성">적색왜성</a> <a href="/wiki/%EC%84%BC%ED%83%80%EC%9A%B0%EB%A3%A8%EC%8A%A4%EC%9E%90%EB%A6%AC_%ED%94%84%EB%A1%9D%EC%8B%9C%EB%A7%88" title="센타우루스자리 프록시마">프록시마</a>가 멀리서 돌고 있는 형태이다. A와 B는 근접거리 11<a href="/wiki/%EC%B2%9C%EB%AC%B8%EB%8B%A8%EC%9C%84" title="천문단위">천문단위</a>, 가장 멀리 떨어질 때 36천문단위의 거리를 보이면서 질량중심을 공전한다. 프록시마는 15,000천문단위 떨어져 있다. 이는 항성과 항성 사이의 거리와 비교할 때는 매우 가깝지만, 중력으로 묶여 있다고 보기에는 먼 거리이기도 하다. 따라서 프록시마와 A,B가 하나의 항성계인지에 대해서는 현재 논란이 있다.</li> <li><a href="/wiki/%ED%8F%B4%EB%9D%BC%EB%A6%AC%EC%8A%A4" title="폴라리스">폴라리스</a>. 삼중성으로, 멀리 떨어진 반성과 매우 가까이 붙어 돌고 있는 분광쌍성이 있다. 이 중 가까운 반성은 <a href="/wiki/2006%EB%85%84" title="2006년">2006년</a> <a href="/wiki/%ED%97%88%EB%B8%94_%EC%9A%B0%EC%A3%BC_%EB%A7%9D%EC%9B%90%EA%B2%BD" class="mw-redirect" title="허블 우주 망원경">허블 우주 망원경</a>이 영상을 분석하여 존재를 알아냈다.</li> <li><a href="/wiki/%EA%B8%80%EB%A6%AC%EC%A0%9C_667" title="글리제 667">글리제 667</a>. 두 개의 K형 주계열성과 적색왜성으로 이뤄진 삼중성계이다. 적색왜성 C는 2개에서 7개 사이의 행성을 보유하고 있으며, 그 중 하나인 Cc는 잠재적으로 거주 가능한 행성이다.</li> <li><a href="/wiki/HD_188753" title="HD 188753">HD 188753</a>은 <a href="/wiki/%EB%B0%B1%EC%A1%B0%EC%9E%90%EB%A6%AC" title="백조자리">백조자리</a>에 있는 삼중성계로 지구에서 149광년 떨어져 있다. 이 계는 HD 188753A(황색 주계열성), HD 188753B(오렌지색 주계열성), HD 188753C(적색왜성) 세 개로 구성되어 있다. B와 C는 서로를 156일에 한 번 공전하며, 이 둘은 한 덩어리가 되어 주성 A 주위를 25.7년에 한 번 공전한다.</li> <li><a href="/wiki/%ED%8F%AC%EB%A7%90%ED%95%98%EC%9A%B0%ED%8A%B8" title="포말하우트">포말하우트</a>는 <a href="/wiki/%EB%82%A8%EC%AA%BD%EB%AC%BC%EA%B3%A0%EA%B8%B0%EC%9E%90%EB%A6%AC" title="남쪽물고기자리">남쪽물고기자리</a>에 있는 삼중성계이다. 2013년 K형 섬광성 <a href="/wiki/%EB%82%A8%EC%AA%BD%EB%AC%BC%EA%B3%A0%EA%B8%B0%EC%9E%90%EB%A6%AC_TW" title="남쪽물고기자리 TW">남쪽물고기자리 TW</a>와 적색왜성 <a href="/w/index.php?title=%ED%8F%AC%EB%A7%90%ED%95%98%EC%9A%B0%ED%8A%B8_C&action=edit&redlink=1" class="new" title="포말하우트 C (없는 문서)">LP 876-10</a>이 우주에서 고유 운동을 공유하는 것이 확인되면서 삼중계로 밝혀졌다. 주성은 초기 태양계와 비슷한 거대한 먼지 원반을 가지고 있지만, 훨씬 더 거대하다. 또한 <a href="/wiki/%EA%B1%B0%EB%8C%80_%EA%B8%B0%EC%B2%B4_%ED%96%89%EC%84%B1" title="거대 기체 행성">거대 기체 행성</a>인 <a href="/wiki/%ED%8F%AC%EB%A7%90%ED%95%98%EC%9A%B0%ED%8A%B8_b" title="포말하우트 b">포말하우트 b</a>를 포함한다. 같은 해, 3차 별인 LP 876-10 역시 먼지 원반을 수용하고 있는 것으로 확인되었다.</li> <li><a href="/w/index.php?title=HD_181068&action=edit&redlink=1" class="new" title="HD 181068 (없는 문서)">HD 181068</a>은 적색거성과 두 개의 주계열성으로 구성된 독특한 삼중계이다. 별의 궤도는 세 별이 모두 서로를 가리는 삼중 식쌍성이다.</li></ul> <div class="mw-heading mw-heading3"><h3 id="사중성계"><span id=".EC.82.AC.EC.A4.91.EC.84.B1.EA.B3.84"></span>사중성계</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=13" title="부분 편집: 사중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/%ED%8C%8C%EC%9D%BC:HD_98800.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/c/c7/HD_98800.jpg/220px-HD_98800.jpg" decoding="async" width="220" height="176" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/c/c7/HD_98800.jpg/330px-HD_98800.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/c/c7/HD_98800.jpg/440px-HD_98800.jpg 2x" data-file-width="3000" data-file-height="2400" /></a><figcaption><a href="/wiki/HD_98800" title="HD 98800">HD 98800</a>은 <a href="/w/index.php?title=%EB%B0%94%EB%8B%A4%EB%B1%80%EC%9E%90%EB%A6%AC_TW_%EC%84%B1%ED%98%91&action=edit&redlink=1" class="new" title="바다뱀자리 TW 성협 (없는 문서)">바다뱀자리 TW 성협</a>에 속한 사중성계이다.</figcaption></figure> <ul><li><a href="/wiki/%EC%B9%B4%ED%8E%A0%EB%9D%BC" title="카펠라">카펠라</a>. 한 쌍의 <a href="/wiki/%EA%B1%B0%EC%84%B1" title="거성">거성</a> 주위를 한 쌍의 <a href="/wiki/%EC%A0%81%EC%83%89%EC%99%9C%EC%84%B1" title="적색왜성">적색왜성</a>이 돌고 있다.</li> <li><a href="/w/index.php?title=%EC%84%BC%ED%83%80%EC%9A%B0%EB%A3%A8%EC%8A%A4%EC%9E%90%EB%A6%AC_4&action=edit&redlink=1" class="new" title="센타우루스자리 4 (없는 문서)">센타우루스자리 4</a><sup id="cite_ref-26" class="reference"><a href="#cite_note-26"><span class="cite-bracket">[</span>26<span class="cite-bracket">]</span></a></sup></li> <li><a href="/wiki/%EC%B9%B4%EB%A9%9C%EB%A0%88%EC%98%A8%EC%9E%90%EB%A6%AC_DI" title="카멜레온자리 DI">카멜레온자리 DI</a></li> <li><a href="/w/index.php?title=%ED%99%A9%EC%86%8C%EC%9E%90%EB%A6%AC_%ED%81%AC%EC%8B%9C&action=edit&redlink=1" class="new" title="황소자리 크시 (없는 문서)">황소자리 크시</a>. 3개의 청백색 K형 주계열성과 1개의 F형 항성으로 이뤄진 사중성계이다. 가까운 궤도를 도는 두 별은 7.15일마다 한 번씩 서로의 주위를 공전한다. 세번째 별은 145일마다 이 두 별 주위 궤도를 돈다. 네 번째 별은 대략 50년마다 다른 세 별의 주위를 돈다.<sup id="cite_ref-Nemravová2013_27-0" class="reference"><a href="#cite_note-Nemravová2013-27"><span class="cite-bracket">[</span>27<span class="cite-bracket">]</span></a></sup></li></ul> <div class="mw-heading mw-heading3"><h3 id="오중성계"><span id=".EC.98.A4.EC.A4.91.EC.84.B1.EA.B3.84"></span>오중성계</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=14" title="부분 편집: 오중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <ul><li><a href="/wiki/%EB%8B%A4%EB%B9%84%ED%9D%90" title="다비흐">다비흐</a>: 최소 다섯 개 별로 이루어져 있음.</li> <li><a href="/wiki/%EB%AF%BC%ED%83%80%EC%B9%B4" title="민타카">민타카</a></li> <li><a href="/wiki/%EC%98%A4%EB%A6%AC%EC%98%A8%EC%9E%90%EB%A6%AC_%EC%8B%9C%EA%B7%B8%EB%A7%88" title="오리온자리 시그마">오리온자리 시그마</a></li> <li><a href="/w/index.php?title=HD_155448&action=edit&redlink=1" class="new" title="HD 155448 (없는 문서)">HD 155448</a><sup id="cite_ref-28" class="reference"><a href="#cite_note-28"><span class="cite-bracket">[</span>28<span class="cite-bracket">]</span></a></sup></li> <li><a href="/w/index.php?title=KIC_4150611&action=edit&redlink=1" class="new" title="KIC 4150611 (없는 문서)">KIC 4150611</a><sup id="cite_ref-29" class="reference"><a href="#cite_note-29"><span class="cite-bracket">[</span>29<span class="cite-bracket">]</span></a></sup></li> <li><a href="/w/index.php?title=1SWASP_J093010.78%2B533859.5&action=edit&redlink=1" class="new" title="1SWASP J093010.78+533859.5 (없는 문서)">1SWASP J093010.78+533859.5</a><sup id="cite_ref-30" class="reference"><a href="#cite_note-30"><span class="cite-bracket">[</span>30<span class="cite-bracket">]</span></a></sup></li></ul> <div class="mw-heading mw-heading3"><h3 id="육중성계"><span id=".EC.9C.A1.EC.A4.91.EC.84.B1.EA.B3.84"></span>육중성계</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=15" title="부분 편집: 육중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <ul><li><a href="/wiki/%EC%B9%B4%EC%8A%A4%ED%86%A0%EB%A5%B4_(%ED%95%AD%EC%84%B1)" title="카스토르 (항성)">카스토르</a>. 분광쌍성 3개로 이루어진 항성계이다.</li> <li><a href="/w/index.php?title=%ED%81%B0%EB%B6%80%EB%A6%AC%EC%83%88%EC%9E%90%EB%A6%AC_%EB%B2%A0%ED%83%80&action=edit&redlink=1" class="new" title="큰부리새자리 베타 (없는 문서)">큰부리새자리 베타</a><sup id="cite_ref-31" class="reference"><a href="#cite_note-31"><span class="cite-bracket">[</span>31<span class="cite-bracket">]</span></a></sup></li> <li><a href="/w/index.php?title=HD_139691&action=edit&redlink=1" class="new" title="HD 139691 (없는 문서)">HD 139691</a><sup id="cite_ref-ads9731_32-0" class="reference"><a href="#cite_note-ads9731-32"><span class="cite-bracket">[</span>32<span class="cite-bracket">]</span></a></sup></li> <li><a href="/w/index.php?title=TYC_7037-89-1&action=edit&redlink=1" class="new" title="TYC 7037-89-1 (없는 문서)">TYC 7037-89-1</a><sup id="cite_ref-33" class="reference"><a href="#cite_note-33"><span class="cite-bracket">[</span>33<span class="cite-bracket">]</span></a></sup></li> <li><a href="/wiki/%EB%AF%B8%EC%9E%90%EB%A5%B4" title="미자르">미자르</a>. 미자르는 분광쌍성 2개가 서로를 돌고 있는 형태이다. 원래 미자르가 쌍성이라는 사실을 <a href="/wiki/1650%EB%85%84" title="1650년">1650년</a> <a href="/w/index.php?title=%EC%A7%80%EC%98%A4%EB%B0%98%EB%8B%88_%EB%B0%94%ED%8B%B0%EC%8A%A4%ED%83%80_%EB%A6%AC%EC%B9%98%EC%98%AC%EB%A6%AC&action=edit&redlink=1" class="new" title="지오반니 바티스타 리치올리 (없는 문서)">지오반니 바티스타 리치올리</a>가 최초로 밝혀낸 것으로 알려졌으나, 그보다 <a href="/w/index.php?title=%EB%B2%A0%EB%84%A4%ED%85%8C%ED%86%A0_%EC%B9%B4%EC%8A%A4%ED%85%94%EB%A6%AC&action=edit&redlink=1" class="new" title="베네테토 카스텔리 (없는 문서)">베네테토 카스텔리</a>와 <a href="/wiki/%EA%B0%88%EB%A6%B4%EB%A0%88%EC%98%A4_%EA%B0%88%EB%A6%B4%EB%A0%88%EC%9D%B4" title="갈릴레오 갈릴레이">갈릴레오 갈릴레이</a>가 먼저 이 사실을 발견했을 가능성이 크다. 이후 A와 B성을 <a href="/wiki/%EB%B6%84%EA%B4%91%ED%95%99" title="분광학">분광학</a>적 방법을 이용하여 관측한 결과, 각각 두 개의 쌍성으로 이루어져서 전체는 4개의 항성으로 이루어진 사중성계임을 알게 되었다. 그런데 2009년 연구결과로 안시쌍성인줄 알았던 <a href="/wiki/%EC%95%8C%EC%BD%94%EB%A5%B4_(%ED%95%AD%EC%84%B1)" title="알코르 (항성)">알코르</a>가 미자르의 중력에 잡혀있다는 것을 알게되었고 알코르 또한 쌍성계임이 밝혀져 전체가 미자르 Aa,Ab,Ba,Bb, 알코르 A,B로 총 육중성계임을 알게 되었다.</li></ul> <div class="mw-heading mw-heading2"><h2 id="칠중성계"><span id=".EC.B9.A0.EC.A4.91.EC.84.B1.EA.B3.84"></span>칠중성계</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=16" title="부분 편집: 칠중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <ul><li><a href="/w/index.php?title=%EC%A0%84%EA%B0%88%EC%9E%90%EB%A6%AC_%EB%88%84&action=edit&redlink=1" class="new" title="전갈자리 누 (없는 문서)">전갈자리 누</a><sup id="cite_ref-34" class="reference"><a href="#cite_note-34"><span class="cite-bracket">[</span>34<span class="cite-bracket">]</span></a></sup></li> <li><a href="/w/index.php?title=%EC%B9%B4%EC%8B%9C%EC%98%A4%ED%8E%98%EC%9D%B4%EC%95%84%EC%9E%90%EB%A6%AC_AR&action=edit&redlink=1" class="new" title="카시오페이아자리 AR (없는 문서)">카시오페이아자리 AR</a><sup id="cite_ref-35" class="reference"><a href="#cite_note-35"><span class="cite-bracket">[</span>35<span class="cite-bracket">]</span></a></sup></li> <li><a href="/w/index.php?title=%EC%84%BC%ED%83%80%EC%9A%B0%EB%A3%A8%EC%8A%A4%EC%9E%90%EB%A6%AC_V871&action=edit&redlink=1" class="new" title="센타우루스자리 V871 (없는 문서)">센타우루스자리 V871</a><sup id="cite_ref-36" class="reference"><a href="#cite_note-36"><span class="cite-bracket">[</span>36<span class="cite-bracket">]</span></a></sup></li></ul> <div class="mw-heading mw-heading2"><h2 id="팔중성계"><span id=".ED.8C.94.EC.A4.91.EC.84.B1.EA.B3.84"></span>팔중성계</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=17" title="부분 편집: 팔중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <ul><li><a href="/wiki/%EC%B9%B4%EC%8B%9C%EC%98%A4%ED%8E%98%EC%9D%B4%EC%95%84%EC%9E%90%EB%A6%AC_%EA%B0%90%EB%A7%88" title="카시오페이아자리 감마">카시오페이아자리 감마</a><sup id="cite_ref-Hutter_37-0" class="reference"><a href="#cite_note-Hutter-37"><span class="cite-bracket">[</span>37<span class="cite-bracket">]</span></a></sup></li></ul> <div class="mw-heading mw-heading2"><h2 id="구중성계"><span id=".EA.B5.AC.EC.A4.91.EC.84.B1.EA.B3.84"></span>구중성계</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=18" title="부분 편집: 구중성계"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <ul><li><a href="/w/index.php?title=%EC%9A%A9%EA%B3%A8%EC%9E%90%EB%A6%AC_QZ&action=edit&redlink=1" class="new" title="용골자리 QZ (없는 문서)">용골자리 QZ</a><sup id="cite_ref-38" class="reference"><a href="#cite_note-38"><span class="cite-bracket">[</span>38<span class="cite-bracket">]</span></a></sup></li></ul> <div class="mw-heading mw-heading2"><h2 id="각주"><span id=".EA.B0.81.EC.A3.BC"></span>각주</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=19" title="부분 편집: 각주"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <style data-mw-deduplicate="TemplateStyles:r35556958">.mw-parser-output .reflist{font-size:90%;margin-bottom:0.5em;list-style-type:decimal}.mw-parser-output .reflist .references{font-size:100%;margin-bottom:0;list-style-type:inherit}.mw-parser-output .reflist-columns-2{column-width:30em}.mw-parser-output .reflist-columns-3{column-width:25em}.mw-parser-output .reflist-columns{margin-top:0.3em}.mw-parser-output .reflist-columns ol{margin-top:0}.mw-parser-output .reflist-columns li{page-break-inside:avoid;break-inside:avoid-column}.mw-parser-output .reflist-upper-alpha{list-style-type:upper-alpha}.mw-parser-output .reflist-upper-roman{list-style-type:upper-roman}.mw-parser-output .reflist-lower-alpha{list-style-type:lower-alpha}.mw-parser-output .reflist-lower-greek{list-style-type:lower-greek}.mw-parser-output .reflist-lower-roman{list-style-type:lower-roman}</style><div class="reflist"> <div class="mw-references-wrap mw-references-columns"><ol class="references"> <li id="cite_note-1"><span class="mw-cite-backlink"><a href="#cite_ref-1">↑</a></span> <span class="reference-text"><cite class="citation web"><a rel="nofollow" class="external text" href="http://www.spacetelescope.org/images/potw1543a/">“Smoke ring for a halo”</a><span class="reference-accessdate">. 2015년 10월 26일에 확인함</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Smoke+ring+for+a+halo&rft_id=http%3A%2F%2Fwww.spacetelescope.org%2Fimages%2Fpotw1543a%2F&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-2"><span class="mw-cite-backlink"><a href="#cite_ref-2">↑</a></span> <span class="reference-text"><a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1968QJRAS...9..388E">Stars of Higher Multiplicity</a>, David S. Evans, <i>Quarterly Journal of the Royal Astronomical Society</i> <b>9</b> (1968), 388–400.</span> </li> <li id="cite_note-toko-3"><span class="mw-cite-backlink"><a href="#cite_ref-toko_3-0">↑</a></span> <span class="reference-text"><a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1997A&AS..124...75T">MSC – a catalogue of physical multiple stars</a>, A. A. Tokovinin, <i>Astronomy and Astrophysics Supplement Series</i> <b>124</b> (July 1997), pp. 75–84.</span> </li> <li id="cite_note-heintz1-4"><span class="mw-cite-backlink"><a href="#cite_ref-heintz1_4-0">↑</a></span> <span class="reference-text"><cite class="citation book">Heintz, W. D. (1978). 《Double Stars》. <a href="/w/index.php?title=D._Reidel&action=edit&redlink=1" class="new" title="D. Reidel (없는 문서)">D. Reidel</a> Publishing Company, Dordrecht. 1쪽. <a href="/wiki/%EA%B5%AD%EC%A0%9C_%ED%91%9C%EC%A4%80_%EB%8F%84%EC%84%9C_%EB%B2%88%ED%98%B8" class="mw-redirect" title="국제 표준 도서 번호">ISBN</a> <a href="/wiki/%ED%8A%B9%EC%88%98:%EC%B1%85%EC%B0%BE%EA%B8%B0/90-277-0885-1" title="특수:책찾기/90-277-0885-1"><bdi>90-277-0885-1</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Double+Stars&rft.pages=1&rft.pub=D.+Reidel+Publishing+Company%2C+Dordrecht&rft.date=1978&rft.isbn=90-277-0885-1&rft.aulast=Heintz&rft.aufirst=W.+D.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-5"><span class="mw-cite-backlink"><a href="#cite_ref-5">↑</a></span> <span class="reference-text"><a rel="nofollow" class="external text" href="http://www.ctio.noao.edu/~atokovin/papers/dynamics.pdf">Dynamics of multiple stars: observations</a> <a rel="nofollow" class="external text" href="https://web.archive.org/web/20060919155603/http://www.ctio.noao.edu/~atokovin/papers/dynamics.pdf#">Archived</a> 2006년 9월 19일 - <a href="/wiki/%EC%9B%A8%EC%9D%B4%EB%B0%B1_%EB%A8%B8%EC%8B%A0" title="웨이백 머신">웨이백 머신</a>, A. Tokovinin, in "Massive Stars in Interacting Binaries", 16–20 August 2004, Quebec (ASP Conf. Ser., in print).</span> </li> <li id="cite_note-6"><span class="mw-cite-backlink"><a href="#cite_ref-6">↑</a></span> <span class="reference-text"><cite class="citation book">Heintz, W. D. (1978). 《Double Stars》. D. Reidel Publishing Company, Dordrecht. 66–67쪽. <a href="/wiki/%EA%B5%AD%EC%A0%9C_%ED%91%9C%EC%A4%80_%EB%8F%84%EC%84%9C_%EB%B2%88%ED%98%B8" class="mw-redirect" title="국제 표준 도서 번호">ISBN</a> <a href="/wiki/%ED%8A%B9%EC%88%98:%EC%B1%85%EC%B0%BE%EA%B8%B0/90-277-0885-1" title="특수:책찾기/90-277-0885-1"><bdi>90-277-0885-1</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Double+Stars&rft.pages=66-67&rft.pub=D.+Reidel+Publishing+Company%2C+Dordrecht&rft.date=1978&rft.isbn=90-277-0885-1&rft.aulast=Heintz&rft.aufirst=W.+D.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-evans-7"><span class="mw-cite-backlink">↑ <sup><a href="#cite_ref-evans_7-0">가</a></sup> <sup><a href="#cite_ref-evans_7-1">나</a></sup></span> <span class="reference-text"><cite class="citation journal">Evans, David S. (1968). “Stars of Higher Multiplicity”. 《Quarterly Journal of the Royal Astronomical Society》 <b>9</b>: 388–400. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1968QJRAS...9..388E">1968QJRAS...9..388E</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Quarterly+Journal+of+the+Royal+Astronomical+Society&rft.atitle=Stars+of+Higher+Multiplicity&rft.volume=9&rft.pages=388-400&rft.date=1968&rft_id=info%3Abibcode%2F1968QJRAS...9..388E&rft.aulast=Evans&rft.aufirst=David+S.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-8"><span class="mw-cite-backlink"><a href="#cite_ref-8">↑</a></span> <span class="reference-text">A Note on the Stability of Hierarchical Triple Stars with Initially Circular Orbits, L. G. Kiseleva, P. P. Eggleton, and J. P. Anosova, <i><a href="/wiki/Monthly_Notices_of_the_Royal_Astronomical_Society" class="mw-redirect" title="Monthly Notices of the Royal Astronomical Society">Monthly Notices of the Royal Astronomical Society</a></i> <b>267</b>, #1 (March 1994), pp. 161–166, <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>: <a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1994MNRAS.267..161K/abstract">1994MNRAS.267..161K</a>.</span> </li> <li id="cite_note-9"><span class="mw-cite-backlink"><a href="#cite_ref-9">↑</a></span> <span class="reference-text">pp. 393–394, <cite class="citation journal">Evans, David S. (1968). “Stars of Higher Multiplicity”. 《Quarterly Journal of the Royal Astronomical Society》 <b>9</b>: 388–400. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1968QJRAS...9..388E">1968QJRAS...9..388E</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Quarterly+Journal+of+the+Royal+Astronomical+Society&rft.atitle=Stars+of+Higher+Multiplicity&rft.volume=9&rft.pages=388-400&rft.date=1968&rft_id=info%3Abibcode%2F1968QJRAS...9..388E&rft.aulast=Evans&rft.aufirst=David+S.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-10"><span class="mw-cite-backlink"><a href="#cite_ref-10">↑</a></span> <span class="reference-text"><cite class="citation book">Heintz, W. D. (1978). 《Double Stars》. D. Reidel Publishing Company, Dordrecht. 72쪽. <a href="/wiki/%EA%B5%AD%EC%A0%9C_%ED%91%9C%EC%A4%80_%EB%8F%84%EC%84%9C_%EB%B2%88%ED%98%B8" class="mw-redirect" title="국제 표준 도서 번호">ISBN</a> <a href="/wiki/%ED%8A%B9%EC%88%98:%EC%B1%85%EC%B0%BE%EA%B8%B0/90-277-0885-1" title="특수:책찾기/90-277-0885-1"><bdi>90-277-0885-1</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Double+Stars&rft.pages=72&rft.pub=D.+Reidel+Publishing+Company%2C+Dordrecht&rft.date=1978&rft.isbn=90-277-0885-1&rft.aulast=Heintz&rft.aufirst=W.+D.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-11"><span class="mw-cite-backlink"><a href="#cite_ref-11">↑</a></span> <span class="reference-text">MSC – a catalogue of physical multiple stars, A. A. Tokovinin, 1997–1999, <a href="/w/index.php?title=Centre_de_Donn%C3%A9es_astronomiques_de_Strasbourg&action=edit&redlink=1" class="new" title="Centre de Données astronomiques de Strasbourg (없는 문서)">CDS</a> ID <a rel="nofollow" class="external text" href="http://cdsarc.u-strasbg.fr/viz-bin/Cat?J/A%2bAS/124/75">J/A+AS/124/75</a>.</span> </li> <li id="cite_note-12"><span class="mw-cite-backlink"><a href="#cite_ref-12">↑</a></span> <span class="reference-text"><cite class="citation journal">Mazeh, Tzevi; 외. (2001). “Studies of multiple stellar systems – IV. The triple-lined spectroscopic system Gliese 644”. 《Monthly Notices of the Royal Astronomical Society》 <b>325</b>: 343–357. <a href="/wiki/ArXiv" title="ArXiv">arXiv</a>:<a rel="nofollow" class="external text" href="//arxiv.org/abs/astro-ph/0102451">astro-ph/0102451</a>. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2001MNRAS.325..343M">2001MNRAS.325..343M</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1046%2Fj.1365-8711.2001.04419.x">10.1046/j.1365-8711.2001.04419.x</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Monthly+Notices+of+the+Royal+Astronomical+Society&rft.atitle=Studies+of+multiple+stellar+systems+%E2%80%93+IV.+The+triple-lined+spectroscopic+system+Gliese+644&rft.volume=325&rft.pages=343-357&rft.date=2001&rft_id=info%3Aarxiv%2Fastro-ph%2F0102451&rft_id=info%3Adoi%2F10.1046%2Fj.1365-8711.2001.04419.x&rft_id=info%3Abibcode%2F2001MNRAS.325..343M&rft.aulast=Mazeh&rft.aufirst=Tzevi&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span>; see §7–8 for a discussion of the quintuple system.</span> </li> <li id="cite_note-13"><span class="mw-cite-backlink"><a href="#cite_ref-13">↑</a></span> <span class="reference-text"><cite class="citation book">Heintz, W. D. (1978). 《Double Stars》. D. Reidel Publishing Company, Dordrecht. 65–66쪽. <a href="/wiki/%EA%B5%AD%EC%A0%9C_%ED%91%9C%EC%A4%80_%EB%8F%84%EC%84%9C_%EB%B2%88%ED%98%B8" class="mw-redirect" title="국제 표준 도서 번호">ISBN</a> <a href="/wiki/%ED%8A%B9%EC%88%98:%EC%B1%85%EC%B0%BE%EA%B8%B0/90-277-0885-1" title="특수:책찾기/90-277-0885-1"><bdi>90-277-0885-1</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Double+Stars&rft.pages=65-66&rft.pub=D.+Reidel+Publishing+Company%2C+Dordrecht&rft.date=1978&rft.isbn=90-277-0885-1&rft.aulast=Heintz&rft.aufirst=W.+D.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-14"><span class="mw-cite-backlink"><a href="#cite_ref-14">↑</a></span> <span class="reference-text"><cite class="citation journal">Harrington, R.S. (1970). “Encounter Phenomena in Triple Stars”. 《Astronomical Journal》 <b>75</b>: 114–118. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1970AJ.....75.1140H">1970AJ.....75.1140H</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1086%2F111067">10.1086/111067</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomical+Journal&rft.atitle=Encounter+Phenomena+in+Triple+Stars&rft.volume=75&rft.pages=114-118&rft.date=1970&rft_id=info%3Adoi%2F10.1086%2F111067&rft_id=info%3Abibcode%2F1970AJ.....75.1140H&rft.aulast=Harrington&rft.aufirst=R.S.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-15"><span class="mw-cite-backlink"><a href="#cite_ref-15">↑</a></span> <span class="reference-text"><cite class="citation journal">Fekel, Francis C (1987). “Multiple stars: Anathemas or friends?”. 《Vistas in Astronomy》 <b>30</b>: 69–76. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1987VA.....30...69F">1987VA.....30...69F</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1016%2F0083-6656%2887%2990021-3">10.1016/0083-6656(87)90021-3</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Vistas+in+Astronomy&rft.atitle=Multiple+stars%3A+Anathemas+or+friends%3F&rft.volume=30&rft.pages=69-76&rft.date=1987&rft_id=info%3Adoi%2F10.1016%2F0083-6656%2887%2990021-3&rft_id=info%3Abibcode%2F1987VA.....30...69F&rft.aulast=Fekel&rft.aufirst=Francis+C&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-16"><span class="mw-cite-backlink"><a href="#cite_ref-16">↑</a></span> <span class="reference-text"><cite class="citation journal">Zhuchkov, R. Ya.; Orlov, V. V.; Rubinov, A. V. (2006). “Multiple stars with low hierarchy: stable or unstable?”. 《Publications of the Astronomical Observatory of Belgrade》 <b>80</b>: 155–160. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2006POBeo..80..155Z">2006POBeo..80..155Z</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Publications+of+the+Astronomical+Observatory+of+Belgrade&rft.atitle=Multiple+stars+with+low+hierarchy%3A+stable+or+unstable%3F&rft.volume=80&rft.pages=155-160&rft.date=2006&rft_id=info%3Abibcode%2F2006POBeo..80..155Z&rft.aulast=Zhuchkov&rft.aufirst=R.+Ya.&rft.au=Orlov%2C+V.+V.&rft.au=Rubinov%2C+A.+V.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-17"><span class="mw-cite-backlink"><a href="#cite_ref-17">↑</a></span> <span class="reference-text"><cite class="citation journal">Rubinov, A. V. (2004). “Dynamical Evolution of Multiple Stars: Influence of the Initial Parameters of the System”. 《Astronomy Reports》 <b>48</b>: 155–160. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2004ARep...48...45R">2004ARep...48...45R</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1134%2F1.1641122">10.1134/1.1641122</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomy+Reports&rft.atitle=Dynamical+Evolution+of+Multiple+Stars%3A+Influence+of+the+Initial+Parameters+of+the+System&rft.volume=48&rft.pages=155-160&rft.date=2004&rft_id=info%3Adoi%2F10.1134%2F1.1641122&rft_id=info%3Abibcode%2F2004ARep...48...45R&rft.aulast=Rubinov&rft.aufirst=A.+V.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-18"><span class="mw-cite-backlink"><a href="#cite_ref-18">↑</a></span> <span class="reference-text"><cite class="citation journal">Harrington, R. S. (1977). “Multiple Star Formation from N-Body System Decay”. 《Rev. Mex. Astron. Astrofis》 <b>3</b>: 209. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1977RMxAA...3..209H">1977RMxAA...3..209H</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Rev.+Mex.+Astron.+Astrofis&rft.atitle=Multiple+Star+Formation+from+N-Body+System+Decay&rft.volume=3&rft.pages=209&rft.date=1977&rft_id=info%3Abibcode%2F1977RMxAA...3..209H&rft.aulast=Harrington&rft.aufirst=R.+S.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-heintztrapezia-19"><span class="mw-cite-backlink">↑ <sup><a href="#cite_ref-heintztrapezia_19-0">가</a></sup> <sup><a href="#cite_ref-heintztrapezia_19-1">나</a></sup></span> <span class="reference-text"><cite class="citation book">Heintz, W. D. (1978). 《Double Stars》. D. Reidel Publishing Company, Dordrecht. 67–68쪽. <a href="/wiki/%EA%B5%AD%EC%A0%9C_%ED%91%9C%EC%A4%80_%EB%8F%84%EC%84%9C_%EB%B2%88%ED%98%B8" class="mw-redirect" title="국제 표준 도서 번호">ISBN</a> <a href="/wiki/%ED%8A%B9%EC%88%98:%EC%B1%85%EC%B0%BE%EA%B8%B0/90-277-0885-1" title="특수:책찾기/90-277-0885-1"><bdi>90-277-0885-1</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Double+Stars&rft.pages=67-68&rft.pub=D.+Reidel+Publishing+Company%2C+Dordrecht&rft.date=1978&rft.isbn=90-277-0885-1&rft.aulast=Heintz&rft.aufirst=W.+D.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-20"><span class="mw-cite-backlink"><a href="#cite_ref-20">↑</a></span> <span class="reference-text">Runaway Stars, Trapezia, and Subtrapezia, Christine Allen, Arcadio Poveda, and Alejandro Hernández-Alcántara, <i>Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias)</i> <b>25</b> (2006), pp. 13–15, <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>: <a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2006RMxAC..25...13A/abstract">2006RMxAC..25...13A</a>.</span> </li> <li id="cite_note-Heintz_1978_68-21"><span class="mw-cite-backlink">↑ <sup><a href="#cite_ref-Heintz_1978_68_21-0">가</a></sup> <sup><a href="#cite_ref-Heintz_1978_68_21-1">나</a></sup></span> <span class="reference-text"><cite class="citation book">Heintz, W. D. (1978). 《Double Stars》. D. Reidel Publishing Company, Dordrecht. 68쪽. <a href="/wiki/%EA%B5%AD%EC%A0%9C_%ED%91%9C%EC%A4%80_%EB%8F%84%EC%84%9C_%EB%B2%88%ED%98%B8" class="mw-redirect" title="국제 표준 도서 번호">ISBN</a> <a href="/wiki/%ED%8A%B9%EC%88%98:%EC%B1%85%EC%B0%BE%EA%B8%B0/90-277-0885-1" title="특수:책찾기/90-277-0885-1"><bdi>90-277-0885-1</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Double+Stars&rft.pages=68&rft.pub=D.+Reidel+Publishing+Company%2C+Dordrecht&rft.date=1978&rft.isbn=90-277-0885-1&rft.aulast=Heintz&rft.aufirst=W.+D.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-Hoogerwerf-22"><span class="mw-cite-backlink"><a href="#cite_ref-Hoogerwerf_22-0">↑</a></span> <span class="reference-text"><cite class="citation journal">Hoogerwerf, R.; de Bruijne, J.H.J.; de Zeeuw, P.T (2000). “The origin of runaway stars”. 《Astrophysical Journal》 <b>544</b> (2): 133–136. <a href="/wiki/ArXiv" title="ArXiv">arXiv</a>:<a rel="nofollow" class="external text" href="//arxiv.org/abs/astro-ph/0007436">astro-ph/0007436</a>. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2000ApJ...544L.133H">2000ApJ...544L.133H</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1086%2F317315">10.1086/317315</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astrophysical+Journal&rft.atitle=The+origin+of+runaway+stars&rft.volume=544&rft.issue=2&rft.pages=133-136&rft.date=2000&rft_id=info%3Aarxiv%2Fastro-ph%2F0007436&rft_id=info%3Adoi%2F10.1086%2F317315&rft_id=info%3Abibcode%2F2000ApJ...544L.133H&rft.aulast=Hoogerwerf&rft.aufirst=R.&rft.au=de+Bruijne%2C+J.H.J.&rft.au=de+Zeeuw%2C+P.T&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-Heintz19-23"><span class="mw-cite-backlink"><a href="#cite_ref-Heintz19_23-0">↑</a></span> <span class="reference-text"><cite class="citation book">Heintz, W. D. (1978). 《Double Stars》. Dordrecht: D. Reidel Publishing Company. 19쪽. <a href="/wiki/%EA%B5%AD%EC%A0%9C_%ED%91%9C%EC%A4%80_%EB%8F%84%EC%84%9C_%EB%B2%88%ED%98%B8" class="mw-redirect" title="국제 표준 도서 번호">ISBN</a> <a href="/wiki/%ED%8A%B9%EC%88%98:%EC%B1%85%EC%B0%BE%EA%B8%B0/90-277-0885-1" title="특수:책찾기/90-277-0885-1"><bdi>90-277-0885-1</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Double+Stars&rft.place=Dordrecht&rft.pages=19&rft.pub=D.+Reidel+Publishing+Company&rft.date=1978&rft.isbn=90-277-0885-1&rft.aulast=Heintz&rft.aufirst=W.+D.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-fmt-24"><span class="mw-cite-backlink">↑ <sup><a href="#cite_ref-fmt_24-0">가</a></sup> <sup><a href="#cite_ref-fmt_24-1">나</a></sup></span> <span class="reference-text"><a rel="nofollow" class="external text" href="http://ad.usno.navy.mil/wds/wdsweb_format.txt">Format, The Washington Double Star Catalog</a> <a rel="nofollow" class="external text" href="https://web.archive.org/web/20080412092018/http://ad.usno.navy.mil/wds/wdsweb_format.txt#">Archived</a> 2008년 4월 12일 - <a href="/wiki/%EC%9B%A8%EC%9D%B4%EB%B0%B1_%EB%A8%B8%EC%8B%A0" title="웨이백 머신">웨이백 머신</a>, Brian D. Mason, Gary L. Wycoff, and William I. Hartkopf, Astrometry Department, <a href="/w/index.php?title=United_States_Naval_Observatory&action=edit&redlink=1" class="new" title="United States Naval Observatory (없는 문서)">United States Naval Observatory</a>. Accessed on line August 20, 2008.</span> </li> <li id="cite_note-25"><span class="mw-cite-backlink"><a href="#cite_ref-25">↑</a></span> <span class="reference-text"><cite class="citation journal">A. A. Tokovinin (July 1997). <a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1997A&AS..124...75T">“MSC – a catalogue of physical multiple stars”</a>. 《Astronomy and Astrophysics Supplement Series》. 124, section 2.4: 75–84. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1997A&AS..124...75T">1997A&AS..124...75T</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1051%2Faas%3A1997181">10.1051/aas:1997181</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomy+and+Astrophysics+Supplement+Series&rft.atitle=MSC+%E2%80%93+a+catalogue+of+physical+multiple+stars&rft.volume=124%2C+section+2.4&rft.pages=75-84&rft.date=1997-07&rft_id=info%3Adoi%2F10.1051%2Faas%3A1997181&rft_id=info%3Abibcode%2F1997A%26AS..124...75T&rft.au=A.+A.+Tokovinin&rft_id=http%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F1997A%26AS..124...75T&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-26"><span class="mw-cite-backlink"><a href="#cite_ref-26">↑</a></span> <span class="reference-text"><a rel="nofollow" class="external text" href="http://www.ctio.noao.edu/~atokovin/stars/index.php?cat=HD&number=120955">4 Centauri</a> <a rel="nofollow" class="external text" href="https://web.archive.org/web/20110615045153/http://www.ctio.noao.edu/~atokovin/stars/index.php?cat=HD&number=120955">보관됨</a> 15 6월 2011 - <a href="/wiki/%EC%9B%A8%EC%9D%B4%EB%B0%B1_%EB%A8%B8%EC%8B%A0" title="웨이백 머신">웨이백 머신</a>, entry in the <a rel="nofollow" class="external text" href="http://www.ctio.noao.edu/~atokovin/stars/">Multiple Star Catalog</a>.</span> </li> <li id="cite_note-Nemravová2013-27"><span class="mw-cite-backlink"><a href="#cite_ref-Nemravová2013_27-0">↑</a></span> <span class="reference-text"><cite class="citation journal">Nemravová, J. A.; 외. (2013). “An Unusual Quadruple System ξ Tauri”. 《Central European Astrophysical Bulletin》 <b>37</b> (1): 207–216. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2013CEAB...37..207N">2013CEAB...37..207N</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Central+European+Astrophysical+Bulletin&rft.atitle=An+Unusual+Quadruple+System+%CE%BE+Tauri&rft.volume=37&rft.issue=1&rft.pages=207-216&rft.date=2013&rft_id=info%3Abibcode%2F2013CEAB...37..207N&rft.aulast=Nemravov%C3%A1&rft.aufirst=J.+A.&rft.au=Harmanec%2C+P.&rft.au=Bencheikh%2C+J.&rft.au=Bolton%2C+C.+T.&rft.au=Bo%C5%BEi%C4%87c%2C+H.&rft.au=Bro%C5%BE%2C+M.&rft.au=Engle%2C+S.&rft.au=Grunhut%2C+J.&rft.au=Guinan%2C+E.+F.&rft.au=Hummel%2C+C.+A.&rft.au=Kor%C4%8D%C3%A1kov%C3%A1%2C+D.&rft.au=Koubsk%C3%BD%2C+P.&rft.au=Mayer%2C+P.&rft.au=Mourard%2C+D.&rft.au=Ribeiro%2C+J.&rft.au=%C5%A0lechta%2C+M.&rft.au=Vokrouhlick%C3%BD%2C+D.&rft.au=Votruba%2C+V.&rft.au=Wolf%2C+M.&rft.au=Zasche%2C+P.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-28"><span class="mw-cite-backlink"><a href="#cite_ref-28">↑</a></span> <span class="reference-text"><cite class="citation journal">Schütz, O.; Meeus, G.; Carmona, A.; Juhász, A.; Sterzik, M. F. (2011). “The young B-star quintuple system HD 155448”. 《Astronomy and Astrophysics》 <b>533</b>: A54. <a href="/wiki/ArXiv" title="ArXiv">arXiv</a>:<a rel="nofollow" class="external text" href="//arxiv.org/abs/1108.1557">1108.1557</a>. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2011A&A...533A..54S">2011A&A...533A..54S</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1051%2F0004-6361%2F201016396">10.1051/0004-6361/201016396</a>. <a href="/wiki/%EC%8B%9C%EB%A7%A8%ED%8B%B1_%EC%8A%A4%EC%B9%BC%EB%9D%BC" title="시맨틱 스칼라">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:56143776">56143776</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomy+and+Astrophysics&rft.atitle=The+young+B-star+quintuple+system+HD+155448&rft.volume=533&rft.pages=A54&rft.date=2011&rft_id=info%3Aarxiv%2F1108.1557&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A56143776&rft_id=info%3Adoi%2F10.1051%2F0004-6361%2F201016396&rft_id=info%3Abibcode%2F2011A%26A...533A..54S&rft.au=Sch%C3%BCtz%2C+O.&rft.au=Meeus%2C+G.&rft.au=Carmona%2C+A.&rft.au=Juh%C3%A1sz%2C+A.&rft.au=Sterzik%2C+M.+F.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-29"><span class="mw-cite-backlink"><a href="#cite_ref-29">↑</a></span> <span class="reference-text"><cite class="citation journal">Gregg, T. A.; Prsa, A.; Welsh, W. F.; Orosz, J. A.; Fetherolf, T. (2013). “A Syzygy of KIC 4150611”. 《American Astronomical Society》 <b>221</b>: 142.12. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2013AAS...22114212G">2013AAS...22114212G</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=American+Astronomical+Society&rft.atitle=A+Syzygy+of+KIC+4150611&rft.volume=221&rft.pages=142.12&rft.date=2013&rft_id=info%3Abibcode%2F2013AAS...22114212G&rft.au=Gregg%2C+T.+A.&rft.au=Prsa%2C+A.&rft.au=Welsh%2C+W.+F.&rft.au=Orosz%2C+J.+A.&rft.au=Fetherolf%2C+T.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-30"><span class="mw-cite-backlink"><a href="#cite_ref-30">↑</a></span> <span class="reference-text"><cite class="citation journal">Lohr, M. E.; 외. (2015). “The doubly eclipsing quintuple low-mass star system 1SWASP J093010.78+533859.5”. 《Astronomy & Astrophysics》 <b>578</b>: A103. <a href="/wiki/ArXiv" title="ArXiv">arXiv</a>:<a rel="nofollow" class="external text" href="//arxiv.org/abs/1504.07065">1504.07065</a>. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2015A&A...578A.103L">2015A&A...578A.103L</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1051%2F0004-6361%2F201525973">10.1051/0004-6361/201525973</a>. <a href="/wiki/%EC%8B%9C%EB%A7%A8%ED%8B%B1_%EC%8A%A4%EC%B9%BC%EB%9D%BC" title="시맨틱 스칼라">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:44548756">44548756</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomy+%26+Astrophysics&rft.atitle=The+doubly+eclipsing+quintuple+low-mass+star+system+1SWASP+J093010.78%2B533859.5&rft.volume=578&rft.pages=A103&rft.date=2015&rft_id=info%3Aarxiv%2F1504.07065&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A44548756&rft_id=info%3Adoi%2F10.1051%2F0004-6361%2F201525973&rft_id=info%3Abibcode%2F2015A%26A...578A.103L&rft.au=Lohr%2C+M.+E.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-31"><span class="mw-cite-backlink"><a href="#cite_ref-31">↑</a></span> <span class="reference-text"><cite class="citation web"><a rel="nofollow" class="external text" href="https://web.archive.org/web/20160303233838/http://www.ctio.noao.edu/~atokovin/stars/index.php?ids=00316-6258">“Multiple Star Catalog (MSC)”</a>. 2016년 3월 3일에 <a rel="nofollow" class="external text" href="http://www.ctio.noao.edu/~atokovin/stars/index.php?ids=00316-6258">원본 문서</a>에서 보존된 문서<span class="reference-accessdate">. 2012년 12월 23일에 확인함</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Multiple+Star+Catalog+%28MSC%29&rft_id=http%3A%2F%2Fwww.ctio.noao.edu%2F~atokovin%2Fstars%2Findex.php%3Fids%3D00316-6258&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-ads9731-32"><span class="mw-cite-backlink"><a href="#cite_ref-ads9731_32-0">↑</a></span> <span class="reference-text"><cite class="citation journal">Tokovinin, A. A.; Shatskii, N. I.; Magnitskii, A. K. (1998). “ADS 9731: A new sextuple system”. 《Astronomy Letters》 <b>24</b> (6): 795. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/1998AstL...24..795T">1998AstL...24..795T</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomy+Letters&rft.atitle=ADS+9731%3A+A+new+sextuple+system&rft.volume=24&rft.issue=6&rft.pages=795&rft.date=1998&rft_id=info%3Abibcode%2F1998AstL...24..795T&rft.aulast=Tokovinin&rft.aufirst=A.+A.&rft.au=Shatskii%2C+N.+I.&rft.au=Magnitskii%2C+A.+K.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-33"><span class="mw-cite-backlink"><a href="#cite_ref-33">↑</a></span> <span class="reference-text"><cite class="citation web">Md, By Jeanette Kazmierczak NASA's Goddard Space Flight Center, Greenbelt. <a rel="nofollow" class="external text" href="https://exoplanets.nasa.gov/news/1672/discovery-alert-first-six-star-system-where-all-six-stars-undergo-eclipses/">“Discovery Alert: First Six-star System Where All Six Stars Undergo Eclipses”</a>. 《Exoplanet Exploration: Planets Beyond our Solar System》<span class="reference-accessdate">. 2022년 6월 29일에 확인함</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=unknown&rft.jtitle=Exoplanet+Exploration%3A+Planets+Beyond+our+Solar+System&rft.atitle=Discovery+Alert%3A+First+Six-star+System+Where+All+Six+Stars+Undergo+Eclipses&rft.aulast=Md&rft.aufirst=By+Jeanette+Kazmierczak+NASA%27s+Goddard+Space+Flight+Center%2C+Greenbelt&rft_id=https%3A%2F%2Fexoplanets.nasa.gov%2Fnews%2F1672%2Fdiscovery-alert-first-six-star-system-where-all-six-stars-undergo-eclipses%2F&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-34"><span class="mw-cite-backlink"><a href="#cite_ref-34">↑</a></span> <span class="reference-text"><a rel="nofollow" class="external text" href="http://www.ctio.noao.edu/~atokovin/stars/stars.php?cat=HD&number=145501">Nu Scorpii</a> <a rel="nofollow" class="external text" href="https://web.archive.org/web/20200410223657/http://www.ctio.noao.edu/~atokovin/stars/stars.php?cat=HD&number=145501">보관됨</a> 10 4월 2020 - <a href="/wiki/%EC%9B%A8%EC%9D%B4%EB%B0%B1_%EB%A8%B8%EC%8B%A0" title="웨이백 머신">웨이백 머신</a>, entry in the <a rel="nofollow" class="external text" href="http://www.ctio.noao.edu/~atokovin/stars/">Multiple Star Catalog</a>.</span> </li> <li id="cite_note-35"><span class="mw-cite-backlink"><a href="#cite_ref-35">↑</a></span> <span class="reference-text"><a rel="nofollow" class="external text" href="http://www.ctio.noao.edu/~atokovin/stars/stars.php?cat=HIP&number=115990">AR Cassiopeiae</a> <a rel="nofollow" class="external text" href="https://web.archive.org/web/20200410225127/http://www.ctio.noao.edu/~atokovin/stars/stars.php?cat=HIP&number=115990">보관됨</a> 10 4월 2020 - <a href="/wiki/%EC%9B%A8%EC%9D%B4%EB%B0%B1_%EB%A8%B8%EC%8B%A0" title="웨이백 머신">웨이백 머신</a>, entry in the <a rel="nofollow" class="external text" href="http://www.ctio.noao.edu/~atokovin/stars/">Multiple Star Catalog</a>.</span> </li> <li id="cite_note-36"><span class="mw-cite-backlink"><a href="#cite_ref-36">↑</a></span> <span class="reference-text"><cite class="citation journal">Zasche, P.; Henzl, Z.; Mašek, M. (2022). “Multiply eclipsing candidates from the TESS satellite”. 《Astronomy & Astrophysics》 <b>664</b>: A96. <a href="/wiki/ArXiv" title="ArXiv">arXiv</a>:<a rel="nofollow" class="external text" href="//arxiv.org/abs/2205.03934">2205.03934</a>. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2022A&A...664A..96Z">2022A&A...664A..96Z</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1051%2F0004-6361%2F202243723">10.1051/0004-6361/202243723</a>. <a href="/wiki/%EC%8B%9C%EB%A7%A8%ED%8B%B1_%EC%8A%A4%EC%B9%BC%EB%9D%BC" title="시맨틱 스칼라">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:248571745">248571745</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomy+%26+Astrophysics&rft.atitle=Multiply+eclipsing+candidates+from+the+TESS+satellite&rft.volume=664&rft.pages=A96&rft.date=2022&rft_id=info%3Aarxiv%2F2205.03934&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A248571745&rft_id=info%3Adoi%2F10.1051%2F0004-6361%2F202243723&rft_id=info%3Abibcode%2F2022A%26A...664A..96Z&rft.aulast=Zasche&rft.aufirst=P.&rft.au=Henzl%2C+Z.&rft.au=Ma%C5%A1ek%2C+M.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-Hutter-37"><span class="mw-cite-backlink"><a href="#cite_ref-Hutter_37-0">↑</a></span> <span class="reference-text"><cite class="citation journal">Hutter, D. J.; Tycner, C.; Zavala, R. T.; Benson, J. A.; Hummel, C. A.; Zirm, H. (2021). “Surveying the Bright Stars by Optical Interferometry. III. A Magnitude-limited Multiplicity Survey of Classical Be Stars”. 《The Astrophysical Journal Supplement Series》 <b>257</b> (2): 69. <a href="/wiki/ArXiv" title="ArXiv">arXiv</a>:<a rel="nofollow" class="external text" href="//arxiv.org/abs/2109.06839">2109.06839</a>. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2021ApJS..257...69H">2021ApJS..257...69H</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.3847%2F1538-4365%2Fac23cb">10.3847/1538-4365/ac23cb</a>. <a href="/wiki/%EC%8B%9C%EB%A7%A8%ED%8B%B1_%EC%8A%A4%EC%B9%BC%EB%9D%BC" title="시맨틱 스칼라">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:237503492">237503492</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=The+Astrophysical+Journal+Supplement+Series&rft.atitle=Surveying+the+Bright+Stars+by+Optical+Interferometry.+III.+A+Magnitude-limited+Multiplicity+Survey+of+Classical+Be+Stars&rft.volume=257&rft.issue=2&rft.pages=69&rft.date=2021&rft_id=info%3Aarxiv%2F2109.06839&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A237503492&rft_id=info%3Adoi%2F10.3847%2F1538-4365%2Fac23cb&rft_id=info%3Abibcode%2F2021ApJS..257...69H&rft.aulast=Hutter&rft.aufirst=D.+J.&rft.au=Tycner%2C+C.&rft.au=Zavala%2C+R.+T.&rft.au=Benson%2C+J.+A.&rft.au=Hummel%2C+C.+A.&rft.au=Zirm%2C+H.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> <li id="cite_note-38"><span class="mw-cite-backlink"><a href="#cite_ref-38">↑</a></span> <span class="reference-text"><cite class="citation journal">Mayer, P.; Harmanec, P.; Zasche, P.; Brož, M.; Catalan-Hurtado, R.; Barlow, B. N.; Frondorf, W.; Wolf, M.; Drechsel, H.; Chini, R.; Nasseri, A.; Pigulski, A.; Labadie-Bartz, J.; Christie, G. W.; Walker, W. S. G.; Blackford, M.; Blane, D.; Henden, A. A.; Bohlsen, T.; Božić, H.; Jonák, J. (2022). “Towards a consistent model of the hot quadruple system HD 93206 = QZ Carinæ — I. Observations and their initial analyses”. 《Astronomy & Astrophysics》 <b>666</b>: A23. <a href="/wiki/ArXiv" title="ArXiv">arXiv</a>:<a rel="nofollow" class="external text" href="//arxiv.org/abs/2204.07045">2204.07045</a>. <a href="/wiki/%EB%B9%84%EB%B8%8C%EC%BD%94%EB%93%9C" title="비브코드">Bibcode</a>:<a rel="nofollow" class="external text" href="http://adsabs.harvard.edu/abs/2022A&A...666A..23M">2022A&A...666A..23M</a>. <a href="/wiki/%EB%94%94%EC%A7%80%ED%84%B8_%EA%B0%9D%EC%B2%B4_%EC%8B%9D%EB%B3%84%EC%9E%90" title="디지털 객체 식별자">doi</a>:<a rel="nofollow" class="external text" href="https://dx.doi.org/10.1051%2F0004-6361%2F202142108">10.1051/0004-6361/202142108</a>. <a href="/wiki/%EC%8B%9C%EB%A7%A8%ED%8B%B1_%EC%8A%A4%EC%B9%BC%EB%9D%BC" title="시맨틱 스칼라">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:248177961">248177961</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomy+%26+Astrophysics&rft.atitle=Towards+a+consistent+model+of+the+hot+quadruple+system+HD+93206+%3D+QZ+Carin%C3%A6+%E2%80%94+I.+Observations+and+their+initial+analyses&rft.volume=666&rft.pages=A23&rft.date=2022&rft_id=info%3Aarxiv%2F2204.07045&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A248177961&rft_id=info%3Adoi%2F10.1051%2F0004-6361%2F202142108&rft_id=info%3Abibcode%2F2022A%26A...666A..23M&rft.aulast=Mayer&rft.aufirst=P.&rft.au=Harmanec%2C+P.&rft.au=Zasche%2C+P.&rft.au=Bro%C5%BE%2C+M.&rft.au=Catalan-Hurtado%2C+R.&rft.au=Barlow%2C+B.+N.&rft.au=Frondorf%2C+W.&rft.au=Wolf%2C+M.&rft.au=Drechsel%2C+H.&rft.au=Chini%2C+R.&rft.au=Nasseri%2C+A.&rft.au=Pigulski%2C+A.&rft.au=Labadie-Bartz%2C+J.&rft.au=Christie%2C+G.+W.&rft.au=Walker%2C+W.+S.+G.&rft.au=Blackford%2C+M.&rft.au=Blane%2C+D.&rft.au=Henden%2C+A.+A.&rft.au=Bohlsen%2C+T.&rft.au=Bo%C5%BEi%C4%87%2C+H.&rft.au=Jon%C3%A1k%2C+J.&rfr_id=info%3Asid%2Fko.wikipedia.org%3A%ED%95%AD%EC%84%B1%EA%B3%84" class="Z3988"><span style="display:none;"> </span></span></span> </li> </ol></div></div> <div class="mw-heading mw-heading2"><h2 id="외부_링크"><span id=".EC.99.B8.EB.B6.80_.EB.A7.81.ED.81.AC"></span>외부 링크</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=%ED%95%AD%EC%84%B1%EA%B3%84&action=edit&section=20" title="부분 편집: 외부 링크"><span>편집</span></a><span class="mw-editsection-bracket">]</span></span></div> <ul><li><span typeof="mw:File"><span><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Commons-logo.svg/12px-Commons-logo.svg.png" decoding="async" width="12" height="16" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Commons-logo.svg/18px-Commons-logo.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Commons-logo.svg/24px-Commons-logo.svg.png 2x" data-file-width="1024" data-file-height="1376" /></span></span> 위키미디어 공용에 <span class="plainlinks"><a class="external 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