<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2019-11-20T14:28:49Z" 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>Spectroscopic HR diagram of OB stars in the SMC</title><shortName>J/ApJ/868/57</shortName><identifier>ivo://CDS.VizieR/J/ApJ/868/57</identifier><altIdentifier>doi:10.26093/cds/vizier.18680057</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Castro N.</name></creator><creator><name>Oey M.S.</name></creator><creator><name>Fossati L.</name></creator><creator><name>Langer N.</name></creator><date role="Updated">2020-03-26T14:17:48Z</date><date role="Created">2019-11-20T14:28:49Z</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>magellanic-clouds</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><description>We present a comprehensive stellar atmosphere analysis of 329 O- and B-type stars in the Small Magellanic Cloud (SMC) from the RIOTS4 survey. Using spectroscopically derived effective temperature Teff and surface gravities, we find that classical Be stars appear misplaced to low Teff and high luminosity in the spectroscopic Hertzsprung-Russell diagram (sHRD). Together with the most luminous stars in our sample, the stellar masses derived from the sHRD for these objects are systematically larger than those obtained from the conventional Hertzsprung-Russell diagram. This suggests that the well-known, spectroscopic mass-discrepancy problem may be linked to the fact that both groups of stars have outer envelopes that are nearly gravitationally unbound. The non-emission-line stars in our sample mainly appear on the main sequence, allowing a first estimate of the terminal-age main sequence (TAMS) in the SMC, which matches the predicted TAMS between 12 and 40M_{sun}_ at SMC metallicity. We further find a large underabundance of stars above ~25M_{sun}_ near the zero-age main sequence, reminiscent of such earlier findings in the Milky Way and Large Magellanic Cloud.</description><source format="bibcode">2018ApJ...868...57C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/868/57</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/II/236">II/236 : UBVR CCD survey of the Magellanic clouds (Massey+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/353/601">J/MNRAS/353/601 : 2dF survey of the Small Magellanic Cloud (Evans+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1632">J/AJ/127/1632 : UBVR(UIT) photometry of O and OB stars in SMC (Oey+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/1198">J/ApJ/659/1198 : ARAUCARIA project: NGC 3109 blue supergiants (Evans+, 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/140/416">J/AJ/140/416 : IR photometry of massive stars in the SMC (Bonanos+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A115">J/A+A/530/A115 : Rotating massive MS stars evolutionary models (Brott+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/532/A147">J/A+A/532/A147 : HST photometry in extragalactic star clusters (Larsen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/537/A146">J/A+A/537/A146 : Stellar models with rotation. Z=0.014 (Ekstrom+, 2012)</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/other/Sci/337.444">J/other/Sci/337.444 : RV curves of Galactic massive O stars (Sana+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A103">J/A+A/558/A103 : Stellar models with rotation. Z=0.002 (Georgy+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/442/1680">J/MNRAS/442/1680 : Red giants in SMC. Abundances (Dobbie+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/780/59">J/ApJ/780/59 : The Araucaria project: EBs in SMC (Graczyk+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/591/A11">J/A+A/591/A11 : SMC BV photometry of 9 star cluster fields (Dias+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/113">J/ApJ/817/113 : RIOTS4: spec. survey of SMC field OB stars (Lamb+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/816/49">J/ApJ/816/49 : Spitzer/IRAC observations of SMC Cepheids (Scowcroft+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/600/A81">J/A+A/600/A81 : VLTS. 30Dor O giants &amp; supergiants (Ramirez-Agudelo+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/601/A79">J/A+A/601/A79 : VLTS. O dwarf in 30 Dor (Sabin-Sanjulian+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/597/A22">J/A+A/597/A22 : Massive O- and B-type stars velocities (Simon-Diaz+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/613/A65">J/A+A/613/A65 : Spectroscopic parameters of O-type stars (Holgado+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/867/L8">J/ApJ/867/L8 : Gaia kinematic data of OB stars in SMC (Oey+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Sci/359.69">J/other/Sci/359.69 : Massive stars in 30 Dor (Schneider+, 2018)</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/ApJ/868/57</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/868/57</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/868/57</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/868/57</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/868/57</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/868/57</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/ApJ/868/57/table1 (OB in the SMC analyzed in this work)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/868/57/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/868/57/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/868/57/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>14.1840417</ra><dec>-72.0586944</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/8326 6/33294 33295 33297 33298 33299 33316 33317 33319 33328</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/868/57?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/868/57/table1</name><description>OB in the SMC analyzed in this work</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>ID</name><description>Massey 2002, II/236 identifier; &lt;[M2002] SMC NNNNN&gt; in Simbad</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[0/1] Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[71/73] Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>logTeff</name><description>[4/4.7] log effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logTeff</name><description>[0/0.2] Uncertainty in logTeff</description><unit>log(K)</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLs</name><description>[2.7/4.6] log spectroscopic luminosity (1)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logLs</name><description>[-0/0.7] Uncertainty in logLs</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL</name><description>[0/6] log luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logL</name><description>[0/0.4] Uncertainty in logL</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMsHRD</name><description>[0.7/2]? log estimated mass in the spectroscopic Hertzsprung-Russell diagram (sHRD)(1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logMHRD</name><description>[0.7/1.7]? log estimated mass in the Hertzsprung-Russell diagram (HRD)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Em</name><description>[e] Balmer line emission flag (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Met</name><description>[m] Metals flag (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SCat</name><description>Display data from RIOTS4 (Lamb+, 2016, J/ApJ/817/113); Evans+, 2004, J/MNRAS/353/601 and Bonanos+, 2010, J/AJ/140/416 within 1"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>