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<ri:Resource created="2017-08-23T06:36:31Z" 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>Spitzer h and {chi} Persei candidate members</title><shortName>J/ApJ/796/127</shortName><identifier>ivo://CDS.VizieR/J/ApJ/796/127</identifier><altIdentifier>doi:10.26093/cds/vizier.17960127</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cloutier R.</name></creator><creator><name>Currie T.</name></creator><creator><name>Rieke G.H.</name></creator><creator><name>Kenyon S.J.</name></creator><creator><name>Balog Z.</name></creator><creator><name>Jayawardhana R.</name></creator><date role="Updated">2018-08-24T05:38:26Z</date><date role="Created">2017-08-23T06:36:31Z</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>open-star-clusters</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>line-intensities</subject><description>We analyze very deep Infrared Array Camera and Multiband Imaging Photometer for Spitzer (MIPS) photometry of ~12500 members of the 14 Myr old Double Cluster, h and {chi} Persei, building upon our earlier, shallower Spitzer Cycle 1 studies. Numerous likely members show infrared (IR) excesses at 8 {mu}m and 24 {mu}m, indicative of circumstellar dust. The frequency of stars with 8 {mu}m excess is at least 2% for our entire sample, slightly lower (higher) for B/A stars (later type, lower mass stars). Optical spectroscopy also identifies gas in about 2% of systems, but with no clear trend between the presence of dust and gas. Spectral energy distribution modeling of 18 sources with detections at optical wavelengths through MIPS 24 {mu}m reveals a diverse set of disk evolutionary states, including a high fraction of transitional disks, though similar data for all disk-bearing members would provide constraints. Using Monte Carlo simulations, we combine our results with those for other young clusters to study the global evolution of dust/gas disks. For nominal cluster ages, the e-folding times ({tau}_0_) for the frequency of warm dust and gas are 2.75 Myr and 1.75 Myr, respectively. Assuming a revised set of ages for some clusters, these timescales increase to 5.75 and 3.75 Myr, respectively, implying a significantly longer typical protoplanetary disk lifetime than previously thought. In both cases, the transitional disk duration, averaged over multiple evolutionary pathways, is ~1 Myr. Finally, 24 {mu}m excess frequencies for 4-6 M_{sun}_ stars appear lower than for 1-2.5 M_{sun}_ stars in other 10-30 Myr old clusters.</description><source format="bibcode">2014ApJ...796..127C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/796/127</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/V/27">V/27 : Proper Motions and UBV Photometry in h+chi Per (Muminov 1980)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/122/248">J/AJ/122/248 : h and chi Per UBVI,H{alpha} photometry (Keller+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/576/880">J/ApJ/576/880 : CCD UBV photometry of h and {chi} Per (Slesnick+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/114/233">J/PASP/114/233 : h and {chi} Per memberships (Uribe+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/599">J/ApJ/659/599 : IRAC and JHKs photometry of h and chi Persei (Currie+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/669/L33">J/ApJ/669/L33 : H{alpha} emission sources in h and {chi} Per (Currie+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/672/558">J/ApJ/672/558 : MIPS observations of h and {chi} Persei (Currie+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/191">J/ApJS/186/191 : VI photometry and spectroscopy in h+{chi} Per (Currie+, 2010)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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