<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2021-08-06T10:50:06Z" 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>UKIRT obs. of red supergiants in M31</title><shortName>J/ApJ/889/44</shortName><identifier>ivo://CDS.VizieR/J/ApJ/889/44</identifier><altIdentifier>doi:10.26093/cds/vizier.18890044</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><creator><name>Drout M.R.</name></creator><creator><name>Mommert M.</name></creator><creator><name>Levesque E.M.,Meynet G.</name></creator><creator><name>Ekstrom S.</name></creator><date role="Updated">2022-01-17T11:49:04Z</date><date role="Created">2021-08-06T10:50:06Z</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>infrared-photometry</subject><subject>giant-stars</subject><description>The mass-loss rates of red supergiant stars (RSGs) are poorly constrained by direct measurements, and yet the subsequent evolution of these stars depends critically on how much mass is lost during the RSG phase. In 2012 the Geneva evolutionary group updated their mass-loss prescription for RSGs with the result that a 20M_{sun}_ star now loses 10 times more mass during the RSG phase than in the older models. Thus, higher-mass RSGs evolve back through a second yellow supergiant phase rather than exploding as Type II-P supernovae, in accord with recent observations (the so-called "RSG Problem"). Still, even much larger mass-loss rates during the RSG phase cannot be ruled out by direct measurements of their current dust-production rates, as such mass loss is episodic. Here, we test the models by deriving a luminosity function for RSGs in the nearby spiral galaxy, M31, which is sensitive to the total mass loss during the RSG phase. We carefully separate RSGs from asymptotic giant branch stars in the color-magnitude diagram following the recent method exploited by Yang+ (2019, J/A+A/629/A91) in their Small Magellanic Cloud studies. Comparing our resulting luminosity function with that predicted by the evolutionary models shows that the new prescription for RSG mass loss does an excellent job of matching the observations, and we can readily rule out significantly larger values.</description><source format="bibcode">2020ApJ...889...44N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/889/44</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/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/96/269">J/A+AS/96/269 : Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/333/231">J/A+A/333/231 : O-M stars model atmospheres (Bessell+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/357/225">J/A+A/357/225 : Mass loss of M supergiants (Josselin+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2867">J/AJ/126/2867 : Red supergiants in Magellanic Clouds (Massey+, 2003)</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/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/395/1409">J/MNRAS/395/1409 : Type II-P SN progenitor constraints (Smartt+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/719/1784">J/ApJ/719/1784 : Yellow supergiants in the SMC (Neugent+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/103">J/AJ/142/103 : Cool evolved stars in SAGE-SMC and SAGE-LMC (Boyer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/97">J/ApJ/750/97 : The yellow and red supergiants of M33 (Drout+, 2012)</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/ApJ/749/177">J/ApJ/749/177 : Yellow and red supergiants in the LMC (Neugent+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/133">J/ApJ/758/133 : Metallicity profile of M31 HII regions &amp; PNe (Sanders+, 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/ApJ/826/224">J/ApJ/826/224 : RSG and foreground candidates in M31 (Massey+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/478/3138">J/MNRAS/478/3138 : Cool supergiants in Magellanic Clouds (Davies+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/A12">J/A+A/616/A12 : Gaia DR2 sources in GC and dSph (Gaia Collaboration+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/629/A91">J/A+A/629/A91 : A source catalog for the SMC (Yang+, 2019)</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/889/44</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/889/44</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/889/44</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/889/44</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/889/44</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/889/44</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/889/44/stars (UKIRT photometry M31 fields A and B (Table 2) and control field (Table 3))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/889/44/stars?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/889/44/stars?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/889/44/stars?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>9.46025</ra><dec>40.9951111</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/2622-2623 2666-2667 2705 2707-2710 2713 2716 2752</spatial><spectral>7.952274030004205e-20 1.7798557115773645e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/889/44?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/889/44/stars</name><description>UKIRT photometry M31 fields A and B (Table 2) and control field (Table 3)</description><column><name>Mm</name><description>[0/3]? Membership flag (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></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>Field</name><description>Field A, B or C=control field; column added by CDS</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>[0] Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>[40/42] Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Jmag</name><description>[6.3/20.5] Apparent J band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>[0.001/0.4] The 1{sigma} uncertainty in Jmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ksmag</name><description>[5.3/18.5] Apparent Ks band magnitude (1)</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>[0.001/0.3] The 1{sigma} uncertainty in Ksmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>J-Ks</name><description>[0.5/2] 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>[0.001/0.4] The 1{sigma} 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></table></schema></tableset></ri:Resource>