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<ri:Resource created="2016-03-14T14:55:18Z" 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>Classical and type II Cepheids IR excesses</title><shortName>J/ApJ/813/29</shortName><identifier>ivo://CDS.VizieR/J/ApJ/813/29</identifier><altIdentifier>doi:10.26093/cds/vizier.18130029</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Schmidt E.G.</name></creator><date role="Updated">2017-11-29T11:49:23Z</date><date role="Created">2016-03-14T14:55:18Z</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>variable-stars</subject><subject>infrared-sources</subject><description>Spectral energy distributions for 132 classical and type II Cepheids were searched for evidence of excess flux above the photospheric level in the mid-infrared. Eight of them were found to have unambiguously strong excess emission while a further 13 showed evidence of weak emission. The presence of emission appears to be unrelated to either the pulsational amplitude or the effective temperature while strong emission is limited to stars with periods longer than 11 days, with a single exception. For the stars with strong emission we attempted to fit the energy distribution with a stellar wind model. No acceptable fit could be found for silicate grains. With graphite or iron grains we could only obtain an acceptable fit if the maximum dust temperature was significantly lower than the condensation temperature. We conclude that the excess emission is not evidence of mass loss.</description><source format="bibcode">2015ApJ...813...29S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/813/29</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/B/vsx">B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><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/J/AJ/150/13">J/AJ/150/13 : Cepheid Radial Velocities (CRaV) project (Evans+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/576/A30">J/A+A/576/A30 : NIR light-curve templates for classical Cepheids (Inno+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/61">J/AJ/146/61 : Type II Cepheid candidates. IV. NSVS sources (Schmidt+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/429/385">J/MNRAS/429/385 : Short-period variables near GC (Matsunaga+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/187">J/AJ/142/187 : HST observations of 7 Pop.II variable stars (Benedict+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/53">J/AJ/141/53 : Lick indices of type II Cepheid candidates (Schmidt+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/60/91">J/AcA/60/91 : VI light curves of SMC type II Cepheids (Soszynski+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/2300">J/AJ/139/2300 : BVIc light curves of 3 type II Cepheids (Rabidoux+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/397/933">J/MNRAS/397/933 : LMC type II Cepheids JHKs magnitudes (Matsunaga+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4598">J/AJ/137/4598 : VR light curve of ASAS-North Cepheids (Schmidt+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/665">J/AJ/133/665 : Photometry of type II Cepheid candidates (Schmidt+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/453/155">J/A+A/453/155 : Extended envelopes around Galactic Cepheids II. 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