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<ri:Resource created="2014-01-20T14:43:38Z" 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>The yellow and red supergiants of M33</title><shortName>J/ApJ/750/97</shortName><identifier>ivo://CDS.VizieR/J/ApJ/750/97</identifier><altIdentifier>doi:10.26093/cds/vizier.17500097</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Drout M.R.</name></creator><creator><name>Massey P.</name></creator><creator><name>Meynet G.</name></creator><date role="Updated">2017-06-20T13:17:36Z</date><date role="Created">2014-01-20T14:43:38Z</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>galaxies</subject><subject>visible-astronomy</subject><subject>giant-stars</subject><subject>radial-velocity</subject><description>Yellow and red supergiants are evolved massive stars whose numbers and locations on the Hertzsprung-Russell (H-R) diagram can provide a stringent test for models of massive star evolution. Previous studies have found large discrepancies between the relative number of yellow supergiants (YSGs) observed as a function of mass and those predicted by evolutionary models, while a disagreement between the predicted and observed locations of red supergiants (RSGs) on the H-R diagram was only recently resolved. Here, we extend these studies by examining the YSG and RSG populations of M33. Unfortunately, identifying these stars is difficult as this portion of the color-magnitude diagram is heavily contaminated by foreground dwarfs. We identify the RSGs through a combination of radial velocities and a two-color surface gravity discriminant, and after re-characterizing the rotation curve of M33 with our newly selected RSGs, we identify the YSGs through a combination of radial velocities and the strength of the OI{lambda}7774 triplet. We examine ~1300 spectra in total and identify 121 YSGs (a sample that is unbiased in luminosity above log(L/L_{sun}_)~4.8) and 189 RSGs. After placing these objects on the H-R diagram, we find that the latest generation of Geneva evolutionary tracks shows excellent agreement with the observed locations of our RSGs and YSGs, the observed relative number of YSGs with mass, and the observed RSG upper mass limit.</description><source format="bibcode">2012ApJ...750...97D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/750/97</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/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/749/177">J/ApJ/749/177 : Yellow and red supergiants in the LMC (Neugent+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/411/263">J/MNRAS/411/263 : JHK variable stars in M33 (Javadi+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/441">J/ApJ/703/441 : Yellow supergiants in M31 (Drout+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/420">J/ApJ/703/420 : Red supergiants in M31 (Massey+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/1405">J/MNRAS/371/1405 : Variables in M33 (Hartman+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/2478">J/AJ/131/2478 : M31 and M33 UBVRI photometry (Massey+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/870">J/AJ/121/870 : BVI photometry of Variables in M33 (Macri+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/501/153">J/ApJ/501/153 : VRB photometry of red supergiants (Massey 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/89/85">J/ApJS/89/85 : Blue and red supergiants in M33 (Ivanov+ 1993)</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/750/97</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/750/97</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/750/97</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/750/97</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/750/97</mirrorURL><mirrorURL 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