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<ri:Resource created="2024-09-09T07:41:23Z" 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>B-type stars abundances from LAMOST DR5 LRS sp.</title><shortName>J/ApJ/937/110</shortName><identifier>ivo://CDS.VizieR/J/ApJ/937/110</identifier><altIdentifier>doi:10.26093/cds/vizier.19370110</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liu Z.</name></creator><creator><name>Cui W.</name></creator><creator><name>Liu C.</name></creator><creator><name>Alexeeva S.</name></creator><creator><name>Shi J.</name></creator><creator><name>Zhao G.</name></creator><date role="Updated">2024-11-06T20:27:35Z</date><date role="Created">2024-09-09T07:41:23Z</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>chemical-abundances</subject><subject>b-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>stellar-spectral-types</subject><subject>giant-stars</subject><subject>effective-temperature</subject><description>We present detailed criteria for the classification of subtypes of B-type supergiants and apply them to 97 supergiants chosen manually from the LAMOST DR5 data set. We obtained the physical parameters (effective temperature, surface gravity, projected rotational velocity) and chemical abundances of C and Si for 103 B-type stars, including 62 supergiants. Non-LTE TLUSTY atmospheric models are employed in our analysis. Projected rotational velocities of B-type stars are found to be systematically smaller than those of the old clusters in the Milky Way. The spectral types and luminosity classes of our manually classified B-type stars are consistent with their effective temperatures and surface gravities derived from the model spectral matching method, respectively. The obtained C and Si abundances for most of our B-type stars are subsolar. Our results indicate that a silicon abundance gradient is -0.0419+/-0.0226dex/kpc in the region of 7.1kpc&lt;=Rg&lt;=14.1kpc, which is in agreement with previous studies.</description><source format="bibcode">2022ApJ...937..110L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/937/110</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/III/195">III/195 : Atlas of Optical Spectral Classification OB Stars (Walborn+ 1990)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/274">III/274 : Galactic O-Star Spectroscopic Survey (GOSSS) (Sota+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/164">V/164 : LAMOST DR5 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/156">V/156 : LAMOST DR7 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/434/1125">J/A+A/434/1125 : B-type Supergiants in the SMC (Dufton+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/436/687">J/A+A/436/687 : SMC NGC 346-11 and AV 304 spectra (Hunter+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/809">J/AJ/129/809 : B-star rot. velocities in h and {chi} Persei (Strom+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/457/265">J/A+A/457/265 : The VLT-FLAMES Survey of Massive Stars (Dufton+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/466/277">J/A+A/466/277 : VLT-FLAMES survey of massive stars (Hunter+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/471/625">J/A+A/471/625 : VLT-FLAMES survey of massive stars (Trundle+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1092">J/AJ/133/1092 : vsini of B0-B3 stars in 7 young clusters (Wolff+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/539/A143">J/A+A/539/A143 : Nearby B-stars stellar param. and abundances (Nieva+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A135">J/A+A/562/A135 : Northern Galactic OB stars vsini (Simon-Diaz+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/580/A17">J/A+A/580/A17 : {alpha}-element abundances of Cepheid stars (Genovali+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/603/A91">J/A+A/603/A91 : VLTS. 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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>ObsID</name><description>[5116047/647602217] LAMOST Observation ID (1)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>LAMOST</name><description>LAMOST 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>[13.98/346.14] Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-3.04/58.7] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>S/N</name><description>[16/974] Signal-to-noise ratio at the g-band</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpT</name><description>Spectral type using our criteria</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Teff</name><description>[15/30]? Effective temperature</description><unit>kK</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_Teff</name><description>Flag on Teff (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logg</name><description>[2.25/4]? Log of surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>vsini</name><description>[10/270]? Rotational velocity</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>n_vsini</name><description>The metal line used to obtain vsini</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Vt</name><description>[5/20]? 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