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<ri:Resource created="2014-09-02T12:57:50Z" 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>Wolf-Rayet content of M31</title><shortName>J/ApJ/759/11</shortName><identifier>ivo://CDS.VizieR/J/ApJ/759/11</identifier><altIdentifier>doi:10.26093/cds/vizier.17590011</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Neugent K.F.</name></creator><creator><name>Massey P.</name></creator><creator><name>Georgy C.</name></creator><date role="Updated">2023-04-19T14:25:13Z</date><date role="Created">2014-09-02T12:57:50Z</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>line-intensities</subject><subject>stellar-spectral-types</subject><subject>wolf-rayet-stars</subject><subject>spectroscopy</subject><subject>galaxies</subject><description>Wolf-Rayet (WR) stars are evolved massive stars, and the relative number of WC-type and WN-type WRs should vary with the metallicity of the host galaxy, providing a sensitive test of stellar evolutionary theory. However, past studies of the WR content of M31 have been biased toward detecting WC stars, as their emission-line signatures are much stronger than those of WNs. Here, we present the results of a survey covering all of M31's optical disk (2.2deg^2^), with sufficient sensitivity to detect the weaker-lined WN types. We identify 107 newly found WR stars, mostly of WN type. This brings the total number of spectroscopically confirmed WRs in M31 to 154, a number we argue is complete to ~95%, except in regions of unusually high reddening. This number is consistent with what we expect from the integrated H{alpha} luminosity compared to that of M33. The majority of these WRs formed in OB associations around the Population I ring, although 5% are truly isolated. Both the relative number of WC- to WN-type stars as well as the WC subtype distribution suggest that most WRs exist in environments with higher-than-solar metallicities, which is consistent with studies of M31's metallicity. Although the WC to WN ratio we find for M31 is much lower than that found by previous studies, it is still higher than what the Geneva evolutionary models predict. This may suggest that Roche-lobe overflow produces the excess of WC stars observed at high metallicity, or that the assumed rotational velocities in the models are too high.</description><source format="bibcode">2012ApJ...759...11N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/759/11</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/215">III/215 : 7th Catalog of Galactic Wolf-Rayet stars (van der Hucht, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/143">III/143 : Spectrophotometry of Wolf-Rayet Stars (Torres-Dodgen+ 1988)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/149">J/AJ/143/149 : NIR spectro. of Galactic Wolf-Rayet stars. II. (Shara+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/123">J/ApJ/733/123 : The Wolf-Rayet content of M33 (NGC 598) (Neugent+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A55">J/A+A/534/A55 : Deep XMM-Newton Survey of M31 (Stiele+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A61">J/A+A/509/A61 : Long slit spectroscopy in M31 (Saglia+, 2010)</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/AJ/134/2474">J/AJ/134/2474 : H{alpha} em.-line stars in 7 dwarfs galaxies (Massey+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2393">J/AJ/133/2393 : UBVRI phot. in 7 Local Group dwarfs galaxies (Massey+, 2007)</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/A+A/373/63">J/A+A/373/63 : M31 second ROSAT PSPC survey (Supper+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/505/793">J/ApJ/505/793 : New WR star in M33 (Massey+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/110/2715">J/AJ/110/2715 : UBV photometry in NGC 6822, M31 and M33 (Massey+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/102/251">J/A+AS/102/251 : Objective-prism survey of M31 em. objects (Meyssonnier+ 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/759/11</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/759/11</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/759/11</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/759/11</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/759/11</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/759/11</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/759/11/m31wr (Spectroscopically confirmed M31 WR stars (tables 2 and 5))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/759/11/m31wr?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/759/11/m31wr?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/759/11/m31wr?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>9.7382917</ra><dec>40.5256111</dec><sr>0.005555555555555556</sr></testQuery></capability><capability><description>Associated data</description><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/ApJ/759/11</accessURL></interface></capability><coverage><spatial>6/2622-2623 2666 2708-2709 2752</spatial><spectral>3.322582951404819e-19 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/759/11?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/759/11/m31wr</name><description>Spectroscopically confirmed M31 WR stars (tables 2 and 5)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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