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<ri:Resource created="2026-08-06T17:52:16Z" status="active" updated="2026-08-06T17:00:54Z" 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>Equal-volume radii approx. through Lagrange points</title><shortName>J/A+A/712/A76</shortName><identifier>ivo://CDS.VizieR/J/A+A/712/A76</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Qi S.</name></creator><creator><name>Song H.</name></creator><creator><name>Meynet G.</name></creator><creator><name>Maeder A.</name></creator><creator><name>Ban Z.-L.</name></creator><creator><name>Han Z.</name></creator><creator><name>Li Q.-L.</name></creator><creator><name>He Y.,Qu X.-Y.</name></creator><creator><name>Zhong W.-L.</name></creator><creator><name>Zhan Q.</name></creator><date role="Updated">2026-08-06T17:00:54Z</date><date role="Created">2026-08-06T17:52:16Z</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>multiple-stars</subject><subject>stellar-radii</subject><subject>astronomical-models</subject><description>Accurate Roche-lobe radii are vital for mass transfer and binary evolution modeling. While the Eggleton (1983ApJ...268..368E) formula is widely used for its simplicity and 1% accuracy, observations reveal systematic underestimations in certain mass-ratio ranges - a discrepancy expected within the standard Roche framework. Retaining these standard assumptions, we refined the numerical accuracy using Eggleton's formula as a baseline. Crucially, because Eggleton's model only constrains the inner critical surface (L1), it cannot accommodate over-contact binaries that require outer boundary modeling. By extending numerical integrations to the outer critical surface, we derived a more precise formula for the outer Roche-lobe radii. This provides a more realistic physical representation and is a key improvement in this work. Beyond determining the inner and outer Roche-lobe radii, we also established more precise fitting formulae for the positions of L1, L2, and L3. This study aimed to construct volume-equivalent radii formulae for the equipotential surfaces passing through these three Lagrangian points, providing a more comprehensive tool for binary evolution modeling. Furthermore, observational data of contact binaries covering mass ratios q=M2/M1 from 0 to 20 were utilized for validation. In this work, we defined a spherical coordinate system centered on the primary star (M1) and derived analytical approximations for the positions of the three collinear Lagrangian points (L1, L2, and L3). Furthermore, we proposed a new method to calculate the volume-equivalent radii for L2 and L3. By using the lowest points along the L2 and L3 equipotential surfaces as boundaries, this approach divides the peanut-shaped structure into two components, thereby yielding the corresponding volume-equivalent radii R_L2_ and R_L3_. The improved Roche-lobe radii formulae in this study achieve errors &lt;=0.5% across all mass ratios q. The research results provide a more precise theoretical framework for simulating mass overflow and mass loss through L1, L2 and L3. Determining the positions of the Lagrangian points aims to calculate the Roche potential and investigate mass transfer and loss. These new formulae are applicable to any q with higher precision, and L2, and L3 facilitates the analysis of mass loss through the outer Lagrangian points.</description><source format="bibcode">2026A&amp;A...712A..76Q</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/712/A76</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></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/712/A76</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Bibcode</name><description>ADS Bibcode for the system data source</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>q</name><description>Mass ratio (M1/M2)</description><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>1/q</name><description>Inverse mass ratio (M2/M1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Semi-major axis</description><unit>solRad</unit><ucd>phys.angSize.smajAxis</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>M1</name><description>Mass of the primary component</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>M2</name><description>Mass of the secondary component</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R1</name><description>Observed/Model radius of the primary</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R2</name><description>Observed/Model radius of the secondary</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R1Egg</name><description>Equal-volume radius R1 from Eggleton formula</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R2Egg</name><description>Equal-volume radius R2 from Eggleton formula</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R1Egg</name><description>[] Percentage error of Eggleton R1 approximation</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R2Egg</name><description>[] Percentage error of Eggleton R2 approximation</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R1This</name><description>Equal-volume radius R1 from this work</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R2This</name><description>Equal-volume radius R2 from this work</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R1This</name><description>[] Percentage error of R1 from this work</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R2This</name><description>[] Percentage error of R2 from this work</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>