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<ri:Resource created="2024-05-17T07:20:09Z" 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>30 new Wolf-Rayet stars in M31</title><shortName>J/AJ/166/68</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/68</identifier><altIdentifier>doi:10.26093/cds/vizier.51660068</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Neugent K.F.</name></creator><creator><name>Massey P.</name></creator><date role="Updated">2024-11-06T20:18:57Z</date><date role="Created">2024-05-17T07:20:09Z</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>wolf-rayet-stars</subject><subject>photometry</subject><subject>stellar-spectral-types</subject><description>The evolved massive star populations of the Local Group galaxies are generally thought to be well understood. However, recent work has suggested that the Wolf-Rayet (WR) content of M31 may have been underestimated. We therefore began a pilot project to search for new WRs in M31 and to reexamine the completeness of our previous WR survey, finished almost a decade prior. Our improved imaging data and spectroscopic follow-up confirmed 19 new WRs across three small fields in M31. These newly discovered WRs are generally fainter than the previously known sample due to slightly increased reddening as opposed to intrinsic faintness. From these findings, we estimate that there are another ~60 WRs left to be discovered in M31; however, the overall ratio of WN-type (nitrogen-rich) to WC-type (carbon-rich) WRs remains unchanged with our latest additions to the M31 WR census. We are in the process of extending this pilot WR survey to include the rest of M31, and a more complete population will be detailed in our future work.</description><source format="bibcode">2023AJ....166...68N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/68</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/143">III/143 : Spectrophotometry of Wolf-Rayet Stars (Torres-Dodgen+ 1988)</relatedResource><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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/339/53">J/ApJ/339/53 : Planetary nebulae as standard candles. II. (Ciardullo+, 1989)</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/131/2478">J/AJ/131/2478 : M31 and M33 UBVRI photometry (Massey+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/369/120">J/MNRAS/369/120 : Kinematic survey of planetary nebulae in M31 (Merrett+, 2006)</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/ApJ/759/11">J/ApJ/759/11 : Wolf-Rayet content of M31 (Neugent+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/789/10">J/ApJ/789/10 : M33 WR and Of-type Stars (Neugent+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/62">J/AJ/152/62 : LGGS UBVRI photometry of M31 and M33 stars (Massey+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/863/181">J/ApJ/863/181 : The fifth catalog of LMC Wolf-Rayet stars (Neugent+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/922/177">J/ApJ/922/177 : 2MASS red supergiants in the SMC (Massey+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/79">J/AJ/161/79 : Red supergiant stars in M31 and M33 (Massey+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/664/A93">J/A+A/664/A93 : Northern WNE star spectra (Dsilva+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/259/12">J/ApJS/259/12 : Dust extinction law in nearby galaxies. 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