The CORALIE survey for southern extrasolar planets. XVII. New and updated long period and massive planets

<!DOCTYPE html>     <html class="no-js" lang="en">  <head> <title>The CORALIE survey for southern extrasolar planets. XVII. New and updated long period and massive planets - NASA/ADS</title>  <link rel="apple-touch-icon" sizes="180x180" href="//styles/favicon/apple-touch-icon.png" /> <link rel="icon" type="image/png" sizes="32x32" href="//styles/favicon/favicon-32x32.png" /> <link rel="icon" type="image/png" sizes="16x16" href="//styles/favicon/favicon-16x16.png" /> <link rel="manifest" href="//styles/favicon/site.webmanifest" /> <link rel="mask-icon" href="//styles/favicon/safari-pinned-tab.svg" color="#5bbad5" /> <meta name="apple-mobile-web-app-title" content="NASA ADS" /> <meta name="application-name" content="NASA ADS" /> <meta name="msapplication-TileColor" content="#ffc40d" /> <meta name="theme-color" content="#ffffff" />  <link rel="stylesheet" href="/styles/css/styles.css"> <meta name="robots" content="noarchive"> <link rel="canonical" href="http://ui.adsabs.harvard.edu/abs/2013A&A...551A..90M/abstract"/> <meta name="description" content="Context. Since 1998, a planet-search program around main sequence stars within 50 pc in the southern hemisphere has been carried out with the CORALIE echelle spectrograph at La Silla Observatory. <BR /> Aims: With an observing time span of more than 14 years, the CORALIE survey is now able to unveil Jovian planets on Jupiter's period domain. This growing period-interval coverage is important for building formation and migration models since observational constraints are still weak for periods beyond the ice line. <BR /> Methods: Long-term precise Doppler measurements with the CORALIE echelle spectrograph, together with a few additional observations made with the HARPS spectrograph on the ESO 3.6 m telescope, reveal radial velocity signatures of massive planetary companions on long-period orbits. <BR /> Results: In this paper we present seven new planets orbiting HD 27631, HD 98649, HD 106515A, HD 166724, HD 196067, HD 219077, and HD 220689, together with the CORALIE orbital parameters for three already known planets around HD 10647, HD 30562, and HD 86226. The period range of the new planetary companions goes from 2200 to 5500 days and covers a mass domain between 1 and 10.5 M<SUB>Jup</SUB>. Surprisingly, five of them present very high eccentricities above e &gt; 0.57. A pumping scenario by Kozai mechanism may be invoked for HD 106515Ab and HD 196067b, which are both orbiting stars in multiple systems. Since the presence of a third massive body cannot be inferred from the data of HD 98649b, HD 166724b, and HD 219077b, the origin of the eccentricity of these systems remains unknown. Except for HD 10647b, no constraint on the upper mass of the planets is provided by Hipparcos astrometric data. Finally, the hosts of these long period planets show no metallicity excess. <P />The CORALIE radial velocity measurements discussed in this paper are only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr">cdsarc.u-strasbg.fr</A> (<A href="http://130.79.128.5">130.79.128.5</A>) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/551/A90">http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/551/A90</A>Based on observations collected with the CORALIE echelle spectrograph mounted on the 1.2 m Swiss telescope at La Silla Observatory and with the HARPS spectrograph on the ESO 3.6 m telescope at La Silla (ESO, Chile).">  <meta property="og:type" content="article"> <meta property="og:title" content="The CORALIE survey for southern extrasolar planets. XVII. New and updated long period and massive planets"> <meta property="og:site_name" content="NASA/ADS"> <meta property="og:description" content="Context. Since 1998, a planet-search program around main sequence stars within 50 pc in the southern hemisphere has been carried out with the CORALIE echelle spectrograph at La Silla Observatory. <BR /> Aims: With an observing time span of more than 14 years, the CORALIE survey is now able to unveil Jovian planets on Jupiter's period domain. This growing period-interval coverage is important for building formation and migration models since observational constraints are still weak for periods beyond the ice line. <BR /> Methods: Long-term precise Doppler measurements with the CORALIE echelle spectrograph, together with a few additional observations made with the HARPS spectrograph on the ESO 3.6 m telescope, reveal radial velocity signatures of massive planetary companions on long-period orbits. <BR /> Results: In this paper we present seven new planets orbiting HD 27631, HD 98649, HD 106515A, HD 166724, HD 196067, HD 219077, and HD 220689, together with the CORALIE orbital parameters for three already known planets around HD 10647, HD 30562, and HD 86226. The period range of the new planetary companions goes from 2200 to 5500 days and covers a mass domain between 1 and 10.5 M<SUB>Jup</SUB>. Surprisingly, five of them present very high eccentricities above e &gt; 0.57. A pumping scenario by Kozai mechanism may be invoked for HD 106515Ab and HD 196067b, which are both orbiting stars in multiple systems. Since the presence of a third massive body cannot be inferred from the data of HD 98649b, HD 166724b, and HD 219077b, the origin of the eccentricity of these systems remains unknown. Except for HD 10647b, no constraint on the upper mass of the planets is provided by Hipparcos astrometric data. Finally, the hosts of these long period planets show no metallicity excess. <P />The CORALIE radial velocity measurements discussed in this paper are only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr">cdsarc.u-strasbg.fr</A> (<A href="http://130.79.128.5">130.79.128.5</A>) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/551/A90">http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/551/A90</A>Based on observations collected with the CORALIE echelle spectrograph mounted on the 1.2 m Swiss telescope at La Silla Observatory and with the HARPS spectrograph on the ESO 3.6 m telescope at La Silla (ESO, Chile)."> <meta property="og:url" content="https://ui.adsabs.harvard.edu/abs/2013A&A...551A..90M/abstract"> <meta property="og:image" content="https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg"> <meta property="article:published_time" content="03/2013"> <meta property="article:author" content="Marmier, M."> <meta property="article:author" content="S茅gransan, D."> <meta property="article:author" content="Udry, S."> <meta property="article:author" content="Mayor, M."> <meta property="article:author" content="Pepe, F."> <meta property="article:author" content="Queloz, D."> <meta property="article:author" content="Lovis, C."> <meta property="article:author" content="Naef, D."> <meta property="article:author" content="Santos, N. C."> <meta property="article:author" content="Alonso, R."> <meta property="article:author" content="Alves, S."> <meta property="article:author" content="Berthet, S."> <meta property="article:author" content="Chazelas, B."> <meta property="article:author" content="Demory, B. -O."> <meta property="article:author" content="Dumusque, X."> <meta property="article:author" content="Eggenberger, A."> <meta property="article:author" content="Figueira, P."> <meta property="article:author" content="Gillon, M."> <meta property="article:author" content="Hagelberg, J."> <meta property="article:author" content="Lendl, M."> <meta property="article:author" content="Mardling, R. A."> <meta property="article:author" content="M茅gevand, D."> <meta property="article:author" content="Neveu, M."> <meta property="article:author" content="Sahlmann, J."> <meta property="article:author" content="Sosnowska, D."> <meta property="article:author" content="Tewes, M."> <meta property="article:author" content="Triaud, A. H. M. J.">  <meta name="citation_journal_title" content="Astronomy and Astrophysics"> <meta name="citation_authors" content="Marmier, M.;S茅gransan, D.;Udry, S.;Mayor, M.;Pepe, F.;Queloz, D.;Lovis, C.;Naef, D.;Santos, N. C.;Alonso, R.;Alves, S.;Berthet, S.;Chazelas, B.;Demory, B. -O.;Dumusque, X.;Eggenberger, A.;Figueira, P.;Gillon, M.;Hagelberg, J.;Lendl, M.;Mardling, R. A.;M茅gevand, D.;Neveu, M.;Sahlmann, J.;Sosnowska, D.;Tewes, M.;Triaud, A. H. M. J."> <meta name="citation_title" content="The CORALIE survey for southern extrasolar planets. XVII. New and updated long period and massive planets"> <meta name="citation_date" content="03/2013"> <meta name="citation_volume" content="551"> <meta name="citation_firstpage" content="A90"> <meta name="citation_doi" content="10.1051/0004-6361/201219639"> <meta name="citation_issn" content="0004-6361"> <meta name="citation_language" content="en"> <meta name="citation_keywords" content="planetary systems"> <meta name="citation_keywords" content="binaries: visual"> <meta name="citation_keywords" content="techniques: radial velocities"> <meta name="citation_keywords" content="stars: general"> <meta name="citation_keywords" content="Astrophysics - Earth and Planetary Astrophysics"> <meta name="citation_abstract_html_url" content="https://ui.adsabs.harvard.edu/abs/2013A&A...551A..90M/abstract"> <meta name="citation_publication_date" content="03/2013"> <meta name="citation_pdf_url" content="https://ui.adsabs.harvard.edu/link_gateway/2013A&A...551A..90M/PUB_PDF"> <meta name="citation_arxiv_id" content="arXiv:1211.6444" /> <link title="schema(PRISM)" rel="schema.prism" href="http://prismstandard.org/namespaces/1.2/basic/" /> <meta name="prism.publicationDate" content="03/2013" /> <meta name="prism.publicationName" content="A&A" /> <meta name="prism.issn" content="0004-6361" /> <meta name="prism.volume" content="551" /> <meta name="prism.startingPage" content="A90" /> <link title="schema(DC)" rel="schema.dc" href="http://purl.org/dc/elements/1.1/" /> <meta name="dc.identifier" content="doi:10.1051/0004-6361/201219639" /> <meta name="dc.date" content="03/2013" /> <meta name="dc.source" content="A&A" /> <meta name="dc.title" content="The CORALIE survey for southern extrasolar planets. XVII. New and updated long period and massive planets" /> <meta name="dc.creator" content="Marmier, M."> <meta name="dc.creator" content="S茅gransan, D."> <meta name="dc.creator" content="Udry, S."> <meta name="dc.creator" content="Mayor, M."> <meta name="dc.creator" content="Pepe, F."> <meta name="dc.creator" content="Queloz, D."> <meta name="dc.creator" content="Lovis, C."> <meta name="dc.creator" content="Naef, D."> <meta name="dc.creator" content="Santos, N. C."> <meta name="dc.creator" content="Alonso, R."> <meta name="dc.creator" content="Alves, S."> <meta name="dc.creator" content="Berthet, S."> <meta name="dc.creator" content="Chazelas, B."> <meta name="dc.creator" content="Demory, B. -O."> <meta name="dc.creator" content="Dumusque, X."> <meta name="dc.creator" content="Eggenberger, A."> <meta name="dc.creator" content="Figueira, P."> <meta name="dc.creator" content="Gillon, M."> <meta name="dc.creator" content="Hagelberg, J."> <meta name="dc.creator" content="Lendl, M."> <meta name="dc.creator" content="Mardling, R. A."> <meta name="dc.creator" content="M茅gevand, D."> <meta name="dc.creator" content="Neveu, M."> <meta name="dc.creator" content="Sahlmann, J."> <meta name="dc.creator" content="Sosnowska, D."> <meta name="dc.creator" content="Tewes, M."> <meta name="dc.creator" content="Triaud, A. H. M. J.">  <meta name="twitter:card" content="summary_large_image"/> <meta name="twitter:description" content="Context. Since 1998, a planet-search program around main sequence stars within 50 pc in the southern hemisphere has been carried out with the CORALIE echelle spectrograph at La Silla Observatory. <BR /> Aims: With an observing time span of more than 14 years, the CORALIE survey is now able to unveil Jovian planets on Jupiter's period domain. This growing period-interval coverage is important for building formation and migration models since observational constraints are still weak for periods beyond the ice line. <BR /> Methods: Long-term precise Doppler measurements with the CORALIE echelle spectrograph, together with a few additional observations made with the HARPS spectrograph on the ESO 3.6 m telescope, reveal radial velocity signatures of massive planetary companions on long-period orbits. <BR /> Results: In this paper we present seven new planets orbiting HD 27631, HD 98649, HD 106515A, HD 166724, HD 196067, HD 219077, and HD 220689, together with the CORALIE orbital parameters for three already known planets around HD 10647, HD 30562, and HD 86226. The period range of the new planetary companions goes from 2200 to 5500 days and covers a mass domain between 1 and 10.5 M<SUB>Jup</SUB>. Surprisingly, five of them present very high eccentricities above e &gt; 0.57. A pumping scenario by Kozai mechanism may be invoked for HD 106515Ab and HD 196067b, which are both orbiting stars in multiple systems. Since the presence of a third massive body cannot be inferred from the data of HD 98649b, HD 166724b, and HD 219077b, the origin of the eccentricity of these systems remains unknown. Except for HD 10647b, no constraint on the upper mass of the planets is provided by Hipparcos astrometric data. Finally, the hosts of these long period planets show no metallicity excess. <P />The CORALIE radial velocity measurements discussed in this paper are only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr">cdsarc.u-strasbg.fr</A> (<A href="http://130.79.128.5">130.79.128.5</A>) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/551/A90">http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/551/A90</A>Based on observations collected with the CORALIE echelle spectrograph mounted on the 1.2 m Swiss telescope at La Silla Observatory and with the HARPS spectrograph on the ESO 3.6 m telescope at La Silla (ESO, Chile)."/> <meta name="twitter:title" content="The CORALIE survey for southern extrasolar planets. XVII. 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XVII. New and updated long period and massive planets <a href=""></a> </h2> <div id="authors-and-aff" class="s-authors-and-aff"> <ul class="list-inline"> <li class="author"><a href="/search/?q=author%3A%22Marmier%2C+M.%22">Marmier, M.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22S%C3%A9gransan%2C+D.%22">S茅gransan, D.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Udry%2C+S.%22">Udry, S.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Mayor%2C+M.%22">Mayor, M.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Pepe%2C+F.%22">Pepe, F.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Queloz%2C+D.%22">Queloz, D.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Lovis%2C+C.%22">Lovis, C.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Naef%2C+D.%22">Naef, D.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Santos%2C+N.+C.%22">Santos, N. C.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Alonso%2C+R.%22">Alonso, R.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Alves%2C+S.%22">Alves, S.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Berthet%2C+S.%22">Berthet, S.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Chazelas%2C+B.%22">Chazelas, B.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Demory%2C+B.+-O.%22">Demory, B. -O.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Dumusque%2C+X.%22">Dumusque, X.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Eggenberger%2C+A.%22">Eggenberger, A.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Figueira%2C+P.%22">Figueira, P.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Gillon%2C+M.%22">Gillon, M.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Hagelberg%2C+J.%22">Hagelberg, J.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Lendl%2C+M.%22">Lendl, M.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Mardling%2C+R.+A.%22">Mardling, R. A.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22M%C3%A9gevand%2C+D.%22">M茅gevand, D.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Neveu%2C+M.%22">Neveu, M.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Sahlmann%2C+J.%22">Sahlmann, J.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Sosnowska%2C+D.%22">Sosnowska, D.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Tewes%2C+M.%22">Tewes, M.</a> </li>; <li class="author"><a href="/search/?q=author%3A%22Triaud%2C+A.+H.+M.+J.%22">Triaud, A. H. M. J.</a> </li> </ul> </div> <div class="s-abstract-text"> <h4 class="sr-only">Abstract</h4> <p> Context. Since 1998, a planet-search program around main sequence stars within 50 pc in the southern hemisphere has been carried out with the CORALIE echelle spectrograph at La Silla Observatory. <BR /> Aims: With an observing time span of more than 14 years, the CORALIE survey is now able to unveil Jovian planets on Jupiter's period domain. This growing period-interval coverage is important for building formation and migration models since observational constraints are still weak for periods beyond the ice line. <BR /> Methods: Long-term precise Doppler measurements with the CORALIE echelle spectrograph, together with a few additional observations made with the HARPS spectrograph on the ESO 3.6 m telescope, reveal radial velocity signatures of massive planetary companions on long-period orbits. <BR /> Results: In this paper we present seven new planets orbiting HD 27631, HD 98649, HD 106515A, HD 166724, HD 196067, HD 219077, and HD 220689, together with the CORALIE orbital parameters for three already known planets around HD 10647, HD 30562, and HD 86226. The period range of the new planetary companions goes from 2200 to 5500 days and covers a mass domain between 1 and 10.5 M<SUB>Jup</SUB>. Surprisingly, five of them present very high eccentricities above e > 0.57. A pumping scenario by Kozai mechanism may be invoked for HD 106515Ab and HD 196067b, which are both orbiting stars in multiple systems. Since the presence of a third massive body cannot be inferred from the data of HD 98649b, HD 166724b, and HD 219077b, the origin of the eccentricity of these systems remains unknown. Except for HD 10647b, no constraint on the upper mass of the planets is provided by Hipparcos astrometric data. Finally, the hosts of these long period planets show no metallicity excess. <P />The CORALIE radial velocity measurements discussed in this paper are only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr">cdsarc.u-strasbg.fr</A> (<A href="http://130.79.128.5">130.79.128.5</A>) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/551/A90">http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/551/A90</A>Based on observations collected with the CORALIE echelle spectrograph mounted on the 1.2 m Swiss telescope at La Silla Observatory and with the HARPS spectrograph on the ESO 3.6 m telescope at La Silla (ESO, Chile). </p> </div> <br> <dl class="s-abstract-dl-horizontal"> <dt>Publication:</dt> <dd> <div id="article-publication">Astronomy and Astrophysics</div> </dd> <dt>Pub Date:</dt> <dd>March 2013</dd> <dt>DOI:</dt> <dd> <span> <a href="/link_gateway/2013A&A...551A..90M/doi:10.1051/0004-6361/201219639" target="_blank" rel="noopener">10.1051/0004-6361/201219639</a> <i class="fa fa-external-link"></i> </span> </dd> <dt>arXiv:</dt> <dd> <span> <a href="/link_gateway/2013A&A...551A..90M/arXiv:1211.6444" target="_blank" rel="noopener">arXiv:1211.6444</a> <i class="fa fa-external-link"></i> </span> </dd> <dt>Bibcode:</dt> <dd> <a href="/abs/2013A%26A...551A..90M/abstract"> 2013A&A...551A..90M </a> <i class="icon-help" title="The bibcode is assigned by the ADS as a unique identifier for the paper."></i> </dd> <dt>Keywords:</dt> <dd> <ul class="list-inline"> <li>planetary systems;</li> <li>binaries: visual;</li> <li>techniques: radial velocities;</li> <li>stars: general;</li> <li>Astrophysics - Earth and Planetary Astrophysics</li> </ul> </dd> <dt>E-Print:</dt> <dd> 14 pages, 16 figures, 4 tables, accepted for publication in Astronomy &amp </dd> </dl> </article> </div> <div data-widget="ShowCitations"></div> <div data-widget="ShowReferences"></div> <div data-widget="ShowCoreads"></div> <div data-widget="ShowSimilar"></div> <div data-widget="ShowTableofcontents"></div> <div data-widget="ShowGraphics"></div> <div data-widget="ShowExportcitation" data-origin="abstract"></div> <div data-widget="ShowMetrics" data-allow-redirect="false"></div> <div data-widget="MetaTagsWidget"></div> </div> </div> </div> <div class="s-right-col-container col-xs-12 col-sm-12 col-md-3 col-lg-2 s-right-column" id="right-col-container" > <div data-widget="ShowResources"> <div data-reactroot="" class="s-right-col-widget-container" style="padding: 10px" > <div> <div class="resources__container"> <div class="resources__full__list"> <div class="resources__header__row"> <i class="fa fa-file-text-o" aria-hidden="true"> </i> <div class="resources__header__title">full text sources</div> </div> <div class="resources__content"> <div class="resources__content__title">Publisher</div> <div class="resources__content__links"> <span> <a href="/link_gateway/2013A&A...551A..90M/PUB_PDF" rel="noopener" class="resources__content__link unlock" > <i class="fa fa-file-pdf-o" aria-hidden="true"> </i> </a> <div class="resources__content__link__separator">|</div> </span> <span> <a href="/link_gateway/2013A&A...551A..90M/PUB_HTML" rel="noopener" class="resources__content__link unlock" > <i class="fa fa-file-text" aria-hidden="true"> </i> </a> </span> </div> </div> <div class="resources__content"> <div class="resources__content__title">arXiv</div> <div class="resources__content__links"> <span> <a href="/link_gateway/2013A&A...551A..90M/EPRINT_PDF" rel="noopener" class="resources__content__link unlock" > <i class="fa fa-file-pdf-o" aria-hidden="true"> </i> </a> <div class="resources__content__link__separator">|</div> </span> <span> <a href="/link_gateway/2013A&A...551A..90M/EPRINT_HTML" rel="noopener" class="resources__content__link unlock" > <i class="fa fa-file-text" aria-hidden="true"> </i> </a> </span> </div> </div> </div> <div class="resources__data__list"> <div class="resources__header__row"> <i class="fa fa-database"></i> <div class="resources__header__title">data products</div> </div> <div class="resources__content"> <a href="/link_gateway/2013A&A...551A..90M/SIMBAD" rel="noopener" class="resources__content__link" >SIMBAD (22)</a > <a href="/link_gateway/2013A&A...551A..90M/ESO" rel="noopener" class="resources__content__link" >ESO (3)</a > <a href="/link_gateway/2013A&A...551A..90M/NExScI" rel="noopener" class="resources__content__link" >NExScI (1)</a > </div> </div> </div> <div data-widget="ShowAssociated"> <div data-reactroot="" class="resources__container"> <div class="resources__header__row"> <i class="fa fa-folder-open"></i> <div class="resources__header__title"> Related Materials (15) </div> </div> <div> <div style=" font-size: 1em; 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