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<ri:Resource created="2024-12-30T11:46:43Z" status="active" updated="2025-07-18T20:13:22Z" 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>Red supergiants in M31, M33, SMC and LMC</title><shortName>J/ApJ/942/69</shortName><identifier>ivo://CDS.VizieR/J/ApJ/942/69</identifier><altIdentifier>doi:10.26093/cds/vizier.19420069</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Massey P.</name></creator><creator><name>Neugent K.F.</name></creator><creator><name>Ekstrom S.</name></creator><creator><name>Georgy C.</name></creator><creator><name>Meynet G.</name></creator><date role="Updated">2025-07-18T20:13:22Z</date><date role="Created">2024-12-30T11:46:43Z</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>supergiant-stars</subject><subject>magellanic-clouds</subject><subject>radial-velocity</subject><subject>infrared-photometry</subject><subject>two-color-diagrams</subject><subject>visible-astronomy</subject><subject>stellar-spectral-types</subject><subject>effective-temperature</subject><description>Mass loss in red supergiants (RSGs) is generally recognized to be episodic, but mass-loss prescriptions fail to reflect this. Evolutionary models show that the total amount of mass lost in this phase determines if these stars evolve to warmer temperatures before undergoing core collapse. The current Geneva evolutionary models mimic episodic mass loss by enhancing the quiescent prescription rates whenever the star's outer layers exceed the Eddington luminosity by a large factor. This results in a 20M_{sun}_ model undergoing 10x more mass loss than it would otherwise, but has little effect on models of lower mass. We can test the validity of this approach observationally by measuring the proportion of high-luminosity RSGs to that predicted by the models. To do this, we use our recent luminosity-limited census of RSGs in M31 and M33, making modest improvements to membership, and adopting extinctions based on the recent panchromatic M31 and M33 Hubble surveys. We then compare the proportions of the highest luminosity RSGs found to that predicted by published Geneva models, as well as to a special set of models computed without the enhanced rates. We find good agreement with the models which include the supra-Eddington enhanced mass loss. The models with lower mass-loss rates predict a larger fraction of high-luminosity RSGs than observed, and thus can be ruled out. We also use these improved data to confirm that the upper luminosity limit of RSGs is logL/L_{sun}_~5.4, regardless of metallicity, using our improved data on M31 and M33 plus previous results on the Magellanic Clouds.</description><source format="bibcode">2023ApJ...942...69M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/942/69</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/147">III/147 : Studies of LMC stellar content (Rousseau+ 1978)</relatedResource><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/V/143">V/143 : Revised Bologna Catalog of M31 clusters, V.5 (Galleti+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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LGGS V mag; if any</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SpType</name><description>LGGS Spectral type; if any</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>RVel</name><description>[-584/-35]? Radial velocity from Massey &amp; Evans (2016); if any</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/942/69/table3</name><description>RSGs in M33</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>[1] Hour of Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[30/31] Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Rho</name><description>[0.01/1] Galactocentric distance; R25 radii (1)</description><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>[12.78/17.3] Apparent UKIRT/WFCAM K magnitude (from Massey+ 2021, J/AJ/161/79)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Kmag</name><description>[0.001/0.11] Uncertainty in Kmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>J-Ks</name><description>[0.79/1.5] The (J-Ks) color index</description><unit>mag</unit><ucd>phot.color;em.IR.J;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_J-Ks</name><description>[0.002/0.14] Uncertainty in J-Ks</description><unit>mag</unit><ucd>stat.error;phot.color;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nobs</name><description>[0/15] Number of observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Mm</name><description>[1/2] Membership based upon Gaia (2)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Temp</name><description>[3200/4400] Effective temperature computed using Av=0.80mag (G1)</description><unit>K</unit><ucd>phys.temperature.effective;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LogLum</name><description>[3.95/5.52] Log luminosity computed using Av=0.80mag (G2)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LGGS</name><description>LGGS Name (Massey+ 2006, J/AJ/131/2478); if any</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>Vmag</name><description>[17.28/22.77]? LGGS V mag; if any</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SpType</name><description>LGGS Spectral type; if any</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>RVel</name><description>[-285/-58]? Radial velocity; if any (3)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_RVel</name><description>[:] Uncertainty flag on RVel</description><ucd>meta.code.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RVelExp</name><description>[-263/-100]? Expected radial velocity; if RVel listed</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M21a</name><description>Display data from Massey+ 2021, J/AJ/161/79</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/942/69/table4</name><description>RSGs in the SMC</description><column><name>DEJ2000</name><description>[70/75] Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Ksmag</name><description>[7.42/12.5] Apparent 2MASS Ks magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></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><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>2MASS</name><description>2MASS identifier (JHHMMSSss+DDMMSSs) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</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>SpType</name><description>Spectral Type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>e_Ksmag</name><description>[0.017/0.05] Uncertainty in Ksmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>J-Ks</name><description>[0.70/1.56] The (J-Ks) color index</description><unit>mag</unit><ucd>phot.color;em.IR.J;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_J-Ks</name><description>[0.026/0.08] Uncertainty in J-Ks</description><unit>mag</unit><ucd>stat.error;phot.color;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mm</name><description>[0/2] Membership based upon Gaia (2)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Temp</name><description>[3050/4500] Effective temperature computed assuming Av=0.40mag (G1)</description><unit>K</unit><ucd>phys.temperature.effective;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LogLum</name><description>[3.49/5.5] Log luminosity computed assuming Av=0.40mag (G2)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ref</name><description>[1/14]? Reference for spectral type (3)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>AltName</name><description>Alternative name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>Comm</name><description>Comment</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="30*">char</dataType></column><column><name>M21b</name><description>Display data from Massey+ 2021, J/ApJ/922/177</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/942/69/table5</name><description>RSGs in the LMC</description><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><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>2MASS</name><description>2MASS identifier (JHHMMSSss+DDMMSSs)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>RAJ2000</name><description>[4/5] Hour of Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[65/72] Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Ksmag</name><description>[6.6/12] Apparent 2MASS Ks magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ksmag</name><description>[0.016/0.06] Uncertainty in Ksmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>J-Ks</name><description>[0.79/1.65] The (J-Ks) color index</description><unit>mag</unit><ucd>phot.color;em.IR.J;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_J-Ks</name><description>[0.02/0.1] Uncertainty in J-Ks</description><unit>mag</unit><ucd>stat.error;phot.color;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mm</name><description>[0/2] Membership based upon Gaia (1)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Temp</name><description>[2900/4400] Effective temperature computed assuming Av=0.40mag (G1)</description><unit>K</unit><ucd>phys.temperature.effective;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LogLum</name><description>[3.5/5.6] Log luminosity computed assuming Av=0.40mag (G2)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpType</name><description>Spectral Type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Ref</name><description>[1/24]? Reference for spectral type (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>AltName</name><description>Alternative name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>N20</name><description>Display data from Neugent+ 2020, J/ApJ/900/118</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>