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<ri:Resource created="2019-03-15T10:48:15Z" 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>Tracers of stellar mass-loss. II.</title><shortName>J/ApJ/856/170</shortName><identifier>ivo://CDS.VizieR/J/ApJ/856/170</identifier><altIdentifier>doi:10.26093/cds/vizier.18560170</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gonzalez-Lopezlira R.A.</name></creator><date role="Updated">2019-03-26T13:05:26Z</date><date role="Created">2019-03-15T10:48:15Z</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>stellar-evolutionary-models</subject><subject>stellar-ages</subject><subject>magellanic-clouds</subject><subject>infrared-photometry</subject><subject>open-star-clusters</subject><description>I present integrated colors and surface brightness fluctuation magnitudes in the mid-infrared (IR), derived from stellar population synthesis models that include the effects of the dusty envelopes around thermally pulsing asymptotic giant branch (TP-AGB) stars. The models are based on the Bruzual &amp; Charlot CB* isochrones; they are single-burst, range in age from a few Myr to 14Gyr, and comprise metallicities between Z=0.0001 and Z=0.04. I compare these models to mid-IR data of AGB stars and star clusters in the Magellanic Clouds, and study the effects of varying self-consistently the mass-loss rate, the stellar parameters, and the output spectra of the stars plus their dusty envelopes. I find that models with a higher than fiducial mass-loss rate are needed to fit the mid-IR colors of "extreme" single AGB stars in the Large Magellanic Cloud. Surface brightness fluctuation magnitudes are quite sensitive to metallicity for 4.5{mu}m and longer wavelengths at all stellar population ages, and powerful diagnostics of mass-loss rate in the TP-AGB for intermediate-age populations, between 100Myr and 2-3Gyr.</description><source format="bibcode">2018ApJ...856..170G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/856/170</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/232">III/232 : STELIB -- A library of stellar spectra at R 2000 (Le Borgne+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/531/A165">J/A+A/531/A165 : MILES atmospheric parameters (Prugniel+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/403/1213">J/MNRAS/403/1213 : Tracers of stellar mass-loss. 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(Gonzalez-Lopezlira+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/1243">J/AJ/138/1243 : The star formation history of the LMC (Harris+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/503/913">J/A+A/503/913 : Synthetic spectrophotometry for C-rich giants (Aringer+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4810">J/AJ/137/4810 : LMC-SAGE AGB star candidates (Srinivasan+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/484/815">J/A+A/484/815 : Scaled solar tracks and isochrones (Bertelli+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/2268">J/AJ/132/2268 : SAGE calibration stars (Meixner+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/703">J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/611/270">J/ApJ/611/270 : Magellanic star clusters IR fluctuations (Gonzalez+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1531">J/AJ/127/1531 : Star formation history of SMC (Harris+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/393/167">J/A+A/393/167 : Mean Spectra for upper AGB stars (Lancon+, 2002)</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/856/170</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/856/170</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/856/170</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/856/170</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/856/170</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/856/170</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/856/170/table4 (Individual cluster photometry)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/856/170/table4?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/856/170/table4?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/856/170/table4?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>264.025</ra><dec>-24.5333333</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/8269 8272 8274 8280 6/1071 22574 22702 28776 28779 28866 28906 29204 29205 29209 29211 29214 29215 29235 29240 29241 29248 29351 29362 33042 33047 33052 33053 33073 33075 33080 33093 33094 33100 33103 33104 33105 33106 33108 33112 33113 33124 33125 33127 33137 33138 33140 33287 33294 33295 33297 33304 33306 33307 33316 33317 33328 33329 37538</spatial><spectral>6.772611666688002e-21 6.185923063528282e-20</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/856/170?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/856/170/table4</name><description>Individual cluster photometry</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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