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<ri:Resource created="2025-09-17T14:38:00Z" status="active" updated="2025-10-01T00:00:00Z" 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>Spectroscopic study of OB stars in Carina Arm</title><shortName>J/MNRAS/515/5993</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/515/5993</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Drew J.E.</name></creator><creator><name>Blake-Parsons F.</name></creator><creator><name>Mohr-Smith M.</name></creator><date role="Updated">2025-09-17T14:17:19Z</date><date role="Created">2025-09-17T14:38:00Z</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>milky-way-galaxy</subject><subject>ob-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>astrometry</subject><subject>photometry</subject><subject>effective-temperature</subject><subject>extinction</subject><subject>radial-velocity</subject><subject>trigonometric-parallax</subject><subject>proper-motions</subject><subject>stellar-distance</subject><description>Massive O and early B stars are important markers of recent star formation and exert a significant influence on their environments during their short lives via photoionization and winds and when they explode as supernovae. In the Milky Way, they can be detected at great distances but often lie behind large dust columns, making detection at short wavelengths difficult. In this study, the use of the less extinguished far-red spectrum (8400-8800 {AA}) for radial velocity measurement is examined. Results are reported for a sample of 164 confirmed OB stars within a 2{deg} field positioned on the Carina Arm. Most stars are at distances between 3 and 6 kpc, and Westerlund 2 is at the field edge. The measured radial velocities have errors concentrated in the 3-10 km.s^-1^ range, with a systematic uncertainty of 2-3 km.s^-1^. These are combined with Gaia-mission astrometry to allow full space motions to be constructed. Up to 22 stars are likely to be runaways, although 8 of them are as likely to be interloping (so far undetected) binaries. The mean azimuthal motion of the sample fits in with recent measurements of Galactic disc rotation. In the Galactocentric radial direction, the mean motion indicates modest infall at a speed of ~10 km.s^-1^. This experiment shows that weak Paschen lines in the far-red can yield credible radial velocity determination, offering the prospect of exploring OB-star kinematics over much more of the Galactic disc than has hitherto been possible.</description><source format="bibcode">2022MNRAS.515.5993D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/515/5993</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/MNRAS/465/1807">J/MNRAS/465/1807 : Deep OB star population in Carina (Mohr-Smith+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/341">II/341 : VPHAS+ DR2 survey (Drew+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/485/2312">J/MNRAS/485/2312 : Outer Galactic disk A and F stars space motions</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/885/131">J/ApJ/885/131 : ~200 high-mass SFR plx &amp; proper motion with VLBI</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/450/3855">J/MNRAS/450/3855 : New OB star candidates in Carina Arm (Mohr-Smith+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/508/4952">J/MNRAS/508/4952 : OB stars in Carina Arm (Drew+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/486/1034">J/MNRAS/486/1034 : O stars of the Galactic starburst NGC 3603 (Drew+, 2019)</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/MNRAS/515/5993</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/515/5993</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/515/5993</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/515/5993</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/515/5993</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/515/5993</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/515/5993/tablea1 (Parameters and measurements of our stars sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/515/5993/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/515/5993/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/515/5993/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>155.51034806</ra><dec>-58.04397889</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/9335 6/38018 38024 38026</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/515/5993?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/515/5993/tablea1</name><description>Parameters and measurements of our stars sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000) (RA_J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000) (DEC_J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>pmDE</name><description>Proper motion in declination from Gaia EDR3 (pmDE)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE</name><description>Uncertainty of pmDE (e_pmDE)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pml</name><description>Galactic longitudinal proper motion (pml)</description><unit>mas/yr</unit><ucd>pos.pm;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pml</name><description>Uncertainty of pml (e_pml)</description><unit>mas/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmb</name><description>Galactic latitudinal proper motion (pmb)</description><unit>mas/yr</unit><ucd>pos.pm;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>GLON</name><description>Galactic longitude in IAU 1958 system (GLON)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude in IAU 1958 system (GLAT)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>gmag</name><description>The g band AB magnitude from VPHAS OB star catalogue of Mohr-Smith (2017MNRAS.465.1807M, Cat. J/MNRAS/465/1807) (g)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_gmag</name><description>Mean random error of gmag (e_g)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Teff)</name><description>Estimated median 50th percentile effective temperature from photometry (logTeff)</description><unit>log(K)</unit><ucd>phys.temperature.effective;stat.median;phot</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_log(Teff)</name><description>Upper uncertainty 84th percentile of log (Teff) (eu_logTeff)</description><unit>log(K)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_log(Teff)</name><description>Lower uncertainty 16th percentile of log (Teff) (el_logTeff)</description><unit>log(K)</unit><ucd>stat.error;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>A0</name><description>Estimated median 50th percentile extinction from photometry (A0)</description><unit>mag</unit><ucd>phys.absorption;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_A0</name><description>Upper uncertainty 84th percentile of A0 (eu_A0)</description><unit>mag</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_A0</name><description>Lower uncertainty 16th percentile of A0 (el_A0)</description><unit>mag</unit><ucd>stat.error;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rv</name><description>Estimated median 50th percentile extinction law paremeter from photometry (Rv)</description><ucd>phys.absorption;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Rv</name><description>Upper uncertainty 84th percentile of Rv (eu_Rv)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rv</name><description>Lower uncertainty 16th percentile of Rv (el_Rv)</description><ucd>stat.error;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Teff)sp</name><description>? Estimated median 50th percentile effective temperature from spectroscopy (speclogTeff)</description><unit>log(K)</unit><ucd>phys.temperature.effective;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_log(Teff)sp</name><description>? Upper uncertainty 84th percentile of log(Teff)sp (eu_speclogTeff)</description><unit>log(K)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_log(Teff)sp</name><description>? Lower uncertainty 16th percentile of log(Teff)sp (el_speclogTeff)</description><unit>log(K)</unit><ucd>stat.error;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>log(g)sp</name><description>? Estimated median 50th percentile surface gravity from spectroscopy (logg)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_log(g)sp</name><description>? Upper uncertainty 84th percentile of log(g)sp (eu_logg)</description><unit>log(cm.s**-2)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_log(g)sp</name><description>? Lower uncertainty 16th percentile of log(g)sp (el_logg)</description><unit>log(cm.s**-2)</unit><ucd>stat.error;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>vsini</name><description>? 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