Conditions for Accretion-induced Collapse of White Dwarfs

<!DOCTYPE html>     <html class="no-js" lang="en">  <head> <title>Conditions for Accretion-induced Collapse of White Dwarfs - 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/1991ApJ...367L..19N/abstract"/> <meta name="description" content="Recent discovery of an unexpectedly large number of low-mass binary pulsars (LMBPs) in globular clusters has instigated active discussions on the evolutionary origin of binary pulsars. Prompted by the possibility that at least some of LMBPs originate from accretion-induced collapse (AIC) of white dwarfs, a reexamination is conducted as to whether or not AIC occurs for the new models of O + Ne + Mg white dwarfs and solid C + O white dwarfs that can ignite explosive nuclear burning at significantly lower central densities than in the previous models. Even with low critical densities, AIC is still much more likely than explosion for both types of white dwarfs. Possible regions for AIC are presented in a diagram of mass accretion rate vs initial mass of the white dwarfs.">  <meta property="og:type" content="article"> <meta property="og:title" content="Conditions for Accretion-induced Collapse of White Dwarfs"> <meta property="og:site_name" content="NASA/ADS"> <meta property="og:description" content="Recent discovery of an unexpectedly large number of low-mass binary pulsars (LMBPs) in globular clusters has instigated active discussions on the evolutionary origin of binary pulsars. Prompted by the possibility that at least some of LMBPs originate from accretion-induced collapse (AIC) of white dwarfs, a reexamination is conducted as to whether or not AIC occurs for the new models of O + Ne + Mg white dwarfs and solid C + O white dwarfs that can ignite explosive nuclear burning at significantly lower central densities than in the previous models. Even with low critical densities, AIC is still much more likely than explosion for both types of white dwarfs. Possible regions for AIC are presented in a diagram of mass accretion rate vs initial mass of the white dwarfs."> <meta property="og:url" content="https://ui.adsabs.harvard.edu/abs/1991ApJ...367L..19N/abstract"> <meta property="og:image" content="https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg"> <meta property="article:published_time" content="01/1991"> <meta property="article:author" content="Nomoto, Ken'ichi"> <meta property="article:author" content="Kondo, Yoji">  <meta name="citation_journal_title" content="The Astrophysical Journal"> <meta name="citation_authors" content="Nomoto, Ken'ichi;Kondo, Yoji"> <meta name="citation_title" content="Conditions for Accretion-induced Collapse of White Dwarfs"> <meta name="citation_date" content="01/1991"> <meta name="citation_volume" content="367"> <meta name="citation_firstpage" content="L19"> <meta name="citation_doi" content="10.1086/185922"> <meta name="citation_issn" content="0004-637X"> <meta name="citation_language" content="en"> <meta name="citation_keywords" content="Globular Clusters"> <meta name="citation_keywords" content="Gravitational Collapse"> <meta name="citation_keywords" content="Pulsars"> <meta name="citation_keywords" content="Stellar Evolution"> <meta name="citation_keywords" content="Stellar Mass Accretion"> <meta name="citation_keywords" content="White Dwarf Stars"> <meta name="citation_keywords" content="Binary Stars"> <meta name="citation_keywords" content="Neutron Stars"> <meta name="citation_keywords" content="Stellar Models"> <meta name="citation_keywords" content="X Ray Binaries"> <meta name="citation_keywords" content="Astrophysics"> <meta name="citation_keywords" content="PULSARS"> <meta name="citation_keywords" content="STARS: ACCRETION"> <meta name="citation_keywords" content="STARS: BINARIES"> <meta name="citation_keywords" content="STARS: NEUTRON"> <meta name="citation_keywords" content="STARS: WHITE DWARFS"> <meta name="citation_keywords" content="X-RAYS: BINARIES"> <meta name="citation_abstract_html_url" content="https://ui.adsabs.harvard.edu/abs/1991ApJ...367L..19N/abstract"> <meta name="citation_publication_date" content="01/1991"> <link title="schema(PRISM)" rel="schema.prism" href="http://prismstandard.org/namespaces/1.2/basic/" /> <meta name="prism.publicationDate" content="01/1991" /> <meta name="prism.publicationName" content="ApJL" /> <meta name="prism.issn" content="0004-637X" /> <meta name="prism.volume" content="367" /> <meta name="prism.startingPage" content="L19" /> <link title="schema(DC)" rel="schema.dc" href="http://purl.org/dc/elements/1.1/" /> <meta name="dc.identifier" content="doi:10.1086/185922" /> <meta name="dc.date" content="01/1991" /> <meta name="dc.source" content="ApJL" /> <meta name="dc.title" content="Conditions for Accretion-induced Collapse of White Dwarfs" /> <meta name="dc.creator" content="Nomoto, Ken'ichi"> <meta name="dc.creator" content="Kondo, Yoji">  <meta name="twitter:card" content="summary_large_image"/> <meta name="twitter:description" content="Recent discovery of an unexpectedly large number of low-mass binary pulsars (LMBPs) in globular clusters has instigated active discussions on the evolutionary origin of binary pulsars. Prompted by the possibility that at least some of LMBPs originate from accretion-induced collapse (AIC) of white dwarfs, a reexamination is conducted as to whether or not AIC occurs for the new models of O + Ne + Mg white dwarfs and solid C + O white dwarfs that can ignite explosive nuclear burning at significantly lower central densities than in the previous models. Even with low critical densities, AIC is still much more likely than explosion for both types of white dwarfs. Possible regions for AIC are presented in a diagram of mass accretion rate vs initial mass of the white dwarfs."/> <meta name="twitter:title" content="Conditions for Accretion-induced Collapse of White Dwarfs"/> <meta name="twitter:site" content="@adsabs"/> <meta name="twitter:domain" content="NASA/ADS"/> <meta name="twitter:image:src" content="https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg"/> <meta name="twitter:creator" content="@adsabs"/> <meta charset="utf-8"> <meta name="viewport" content="width=device-width, initial-scale=1, shrink-to-fit=no"> <base href="/"> <style> .btn-full-ads { color: #fff !important; background-color: #1a1a1a !important; border-color: #1a1a1a !important; margin-top: 9px !important; padding-bottom: 10px !important; padding-top: 10px !important; } .btn-full-ads:hover, .btn-full-ads:focus, .btn-full-ads:active, .btn-full-ads.active, .open>.dropdown-toggle.btn-full-ads { color: #000 !important; background-color: #ddd !important; border-color: 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