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<ri:Resource created="2026-03-16T10:35:14Z" status="active" updated="2026-03-16T09:37:28Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>The fate of MS-BD binaries</title><shortName>J/A+A/707/A312</shortName><identifier>ivo://CDS.VizieR/J/A+A/707/A312</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen Z.</name></creator><creator><name>Jin H.</name></creator><creator><name>Ge H.</name></creator><creator><name>Yu C.</name></creator><creator><name>Wang K.</name></creator><creator><name>Chen D.</name></creator><creator><name>Ma B.</name></creator><date role="Updated">2026-03-16T09:37:28Z</date><date role="Created">2026-03-16T10:35:14Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>eclipsing-binary-stars</subject><subject>brown-dwarfs</subject><subject>standard-stars</subject><subject>stellar-masses</subject><subject>orbits</subject><subject>metallicity</subject><subject>astronomical-reference-materials</subject><description>Understanding the survival and orbital evolution of brown dwarf (BD) companions during the post-main-sequence (MS) evolution of their host stars is increasingly important, especially with recent discoveries of many substellar companions around white dwarfs (WDs). We investigate the long-term evolution and final outcomes of BDs orbiting low-mass MS stars as these evolve into WDs. By comparing forward-modeling populations with observed WD-BD binaries, we test evolutionary models and predict the existence of yet-undetected systems. We employ the COMPAS binary population synthesis code to evolve observed MS-BD systems through the post-MS phases of their host stars into the WD stage, tracking orbital changes driven by mass loss, tides, and common-envelope (CE) evolution. Our simulations reproduce a period gap in the distribution of detached WD-BD binaries, consistent with observations. We also identify a boundary separating detached and semi-detached systems on the period-mass diagram, located at orbital periods of ~1-2 hours depending on the BD mass. We predict that a subset of currently known MS-BD binaries will survive post-MS evolution and emerge as detached WD-BD systems, while others will undergo CE evolution and potentially form cataclysmic variables with BD donors. Our results reproduce the observed period gap in WD-BD binaries and provide quantitative predictions for the role of CE efficiency in shaping their distribution. This work predicts that many WD-BD systems remain undetected, motivating targeted searches with microlensing and high-contrast imaging techniques using next-generation large telescopes.</description><source format="bibcode">2026A&amp;A...707A.312C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/707/A312</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/702/A77">J/A+A/702/A77 : Catalog of 9698 planet candidate solar-type hosts</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/702/A4">J/A+A/702/A4 : kappa And JWST/MIRI images (Godoy+, 2025)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/689/A185">J/A+A/689/A185 : JWST/MIRI HR 2562 B images (Godoy+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/688/A120">J/A+A/688/A120 : BD-14 3065b (TOI-4987b) 2D spectra (Subjak+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/680/A16">J/A+A/680/A16 : RV measurements for 12 stars (Unger+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/678/A107">J/A+A/678/A107 : Long-period substellar companions (Philipot+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/678/A93">J/A+A/678/A93 : Multiples among B-stars in Sco-Cen (Gratton+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/674/A114">J/A+A/674/A114 : Southern extrasolar planets CORALIE survey. 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