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<ri:Resource created="2017-09-11T09:44:16Z" 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/IRS debris disk catalog. II.</title><shortName>J/ApJ/798/87</shortName><identifier>ivo://CDS.VizieR/J/ApJ/798/87</identifier><altIdentifier>doi:10.26093/cds/vizier.17980087</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mittal T.</name></creator><creator><name>Chen C.H.</name></creator><creator><name>Jang-Condell H.</name></creator><creator><name>Manoj P.</name></creator><creator><name>Sargent B.A.</name></creator><creator><name>Watson D.M.,Lisse C.M.</name></creator><date role="Updated">2017-10-26T12:15:57Z</date><date role="Created">2017-09-11T09:44:16Z</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-masses</subject><subject>stellar-spectral-types</subject><subject>stellar-ages</subject><subject>stellar-distance</subject><subject>effective-temperature</subject><subject>infrared-photometry</subject><description>During the Spitzer Space Telescope cryogenic mission, astronomers obtained Infrared Spectrograph (IRS) observations of hundreds of debris disk candidates that have been compiled in the Spitzer IRS Debris Disk Catalog (Chen et al. 2014, J/ApJS/211/25). We have discovered 10 and/or 20 {mu}m silicate emission features toward 120 targets in the catalog and modeled the IRS spectra of these sources, consistent with MIPS 70 {mu}m observations, assuming that the grains are composed of silicates (olivine, pyroxene, forsterite, and enstatite) and are located either in a continuous disk with power-law size and surface density distributions or thin rings that are well-characterized using two separate dust grain temperatures. For systems better fit by the continuous disk model, we find that (1) the dust size distribution power-law index is consistent with that expected from a collisional cascade, q=3.5-4.0, with a large number of values outside this range, and (2) the minimum grain size, a_min_, increases with stellar luminosity, L_*_, but the dependence of a_min_ on L_*_ is weaker than expected from radiation pressure alone. In addition, we also find that (3) the crystalline fraction of dust in debris disks evolves as a function of time with a large dispersion in crystalline fractions for stars of any particular stellar age or mass, (4) the disk inner edge is correlated with host star mass, and (5) there exists substantial variation in the properties of coeval disks in Sco-Cen, indicating that the observed variation is probably due to stochasticity and diversity in planet formation.</description><source format="bibcode">2015ApJ...798...87M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/798/87</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/J/ApJ/697/1578">J/ApJ/697/1578 : A debris disk study of Praesepe (Gaspar+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1646">J/ApJ/705/1646 : Debris disks in Upper Sco (Carpenter+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/242">J/ApJS/188/242 : Variations on debris disks. II. (Kenyon+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/738/122">J/ApJ/738/122 : ScoCen debris disks Around F- and G-type stars (Chen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/745/147">J/ApJ/745/147 : Binaries among debris disk stars (Rodriguez+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/133">J/ApJ/756/133 : ScoCen debris disks around B- and A-type stars (Chen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/768/25">J/ApJ/768/25 : Spitzer and Herschel observations of debris disks</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/25">J/ApJS/211/25 : Spitzer/IRS debris disk catalog. I. 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