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<ri:Resource created="2024-05-27T16:38:06Z" status="active" updated="2025-05-19T09:50:00Z" 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>Masses of OB-type stars from LAMOST DR5</title><shortName>J/ApJS/271/15</shortName><identifier>ivo://CDS.VizieR/J/ApJS/271/15</identifier><altIdentifier>doi:10.26093/cds/vizier.22710015</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Huo Z.</name></creator><creator><name>Liu Z.</name></creator><creator><name>Cui W.</name></creator><creator><name>Liu C.</name></creator><creator><name>Liu J.</name></creator><creator><name>Sun M.</name></creator><creator><name>Feng S.</name></creator><creator><name>Li L.</name></creator><date role="Updated">2024-11-06T20:30:56Z</date><date role="Created">2024-05-27T16:38:06Z</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>ob-stars</subject><subject>stellar-masses</subject><subject>stellar-radii</subject><subject>chemical-abundances</subject><description>The measurements of masses and luminosities of massive stars play an important role in understanding the formation and evolution of their host galaxies. In this work, we present the measurement of masses and luminosities of 2946 OB-type stars, including 78 O-type stars and 2868 B-type stars, based on their stellar parameters (effective temperature, surface gravity, and metallicity) and the Padova and Trieste Stellar Evolution Code isochrones model. Our results show that the median mass and luminosity of the 2946 OB-type stars are 5.4M_{sun}_ and log(L/L_{sun}_)=3.2 with median relative errors of 21.4% and 71.1%, respectively. A good agreement between our results estimated by using our method and those derived by using the orbital motions of binary stars from the literature is found for some B-type stars. In addition, we also fit the mass-luminosity relation of B-type stars by using our derived mass and the luminosity from Gaia Data Release 3.</description><source format="bibcode">2024ApJS..271...15H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/271/15</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/VI/96">VI/96 : Evolutionary Sequences (Fagotto+ 1993-96)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/164">V/164 : LAMOST DR5 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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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>LAMOST</name><description>LAMOST DR5 identifier (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-7.5/61] Declination (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>S/N</name><description>[40/999] Signal-to-Noise in the g band of LAMOST spectra</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[15/46.3] Effective temperature (2)</description><unit>kK</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logg</name><description>[2.2/4.6] Log surface gravity (2)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[M/H]</name><description>[-1/0.3] Metallicity (2)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[3/92] Mass calculated using [M/H] (2)</description><unit>solMass</unit><ucd>phys.mass;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>[0.5/106] Uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error;phys.mass;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass2</name><description>[3/53] Mass calculated using solar metallicity</description><unit>solMass</unit><ucd>phys.mass;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass2</name><description>[0.6/32] Uncertainty in Mass2</description><unit>solMass</unit><ucd>stat.error;phys.mass;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL</name><description>[1.99/6.3] Log luminosity calculated using [M/H] (2)</description><unit>log(solLum)</unit><ucd>phys.luminosity;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logL</name><description>[0.2/2.2] Uncertainty in logL</description><unit>log(solLum)</unit><ucd>stat.error;phys.luminosity;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>[1.3/58.3] Radius calculated using [M/H] (2)</description><unit>solRad</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rad</name><description>[0.56/61] Uncertainty in Rad</description><unit>solRad</unit><ucd>stat.error;phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLbol</name><description>[1/4.8]? 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