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<ri:Resource created="2018-05-15T08:38:16Z" 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 obs. of warm dust in 83 debris disks</title><shortName>J/ApJ/845/120</shortName><identifier>ivo://CDS.VizieR/J/ApJ/845/120</identifier><altIdentifier>doi:10.26093/cds/vizier.18450120</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ballering N.P.</name></creator><creator><name>Rieke G.H.</name></creator><creator><name>Su K.Y.L.</name></creator><creator><name>Gaspar A.</name></creator><date role="Updated">2018-06-19T09:01:07Z</date><date role="Created">2018-05-15T08:38:16Z</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>infrared-photometry</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>The architectures of debris disks encode the history of planet formation in these systems. Studies of debris disks via their spectral energy distributions (SEDs) have found infrared excesses arising from cold dust, warm dust, or a combination of the two. The cold outer belts of many systems have been imaged, facilitating their study in great detail. Far less is known about the warm components, including the origin of the dust. The regularity of the disk temperatures indicates an underlying structure that may be linked to the water snow line. If the dust is generated from collisions in an exo-asteroid belt, the dust will likely trace the location of the water snow line in the primordial protoplanetary disk where planetesimal growth was enhanced. If instead the warm dust arises from the inward transport from a reservoir of icy material farther out in the system, the dust location is expected to be set by the current snow line. We analyze the SEDs of a large sample of debris disks with warm components. We find that warm components in single-component systems (those without detectable cold components) follow the primordial snow line rather than the current snow line, so they likely arise from exo-asteroid belts. While the locations of many warm components in two-component systems are also consistent with the primordial snow line, there is more diversity among these systems, suggesting additional effects play a role.</description><source format="bibcode">2017ApJ...845..120B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/845/120</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/AJ/129/1049">J/AJ/129/1049 : mm and sub-mm obs. of solar-type stars (Carpenter+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/620/1010">J/ApJ/620/1010 : Spitzer 24{mu}m photometry of A dwarfs (Rieke+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/452/245">J/A+A/452/245 : Near-IR photometry of PMS stars in rho Oph (Natta+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/636/1098">J/ApJ/636/1098 : Debris disks around solar-type stars (Bryden+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/653/675">J/ApJ/653/675 : Spitzer 24{mu}m photometry of A dwarfs (Su+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/89">J/ApJ/705/89 : IRS spectra of solar-type stars (Lawler+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1226">J/ApJ/705/1226 : Planet-bearing stars in Spitzer (Bryden+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/147">J/ApJ/753/147 : Herschel observations stars in THA (Donaldson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/135">J/AJ/144/135 : Spitzer 24{mu}m obs. of Hipparcos F stars (Mizusawa+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/427/343">J/MNRAS/427/343 : Infrared excesses of Hipparcos stars (McDonald+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/768/25">J/ApJ/768/25 : Spitzer &amp; Herschel obs. of debris disks (Gaspar+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/775/55">J/ApJ/775/55 : Spitzer IR excesses in A-K stars (Ballering+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/555/A11">J/A+A/555/A11 : DUNES survey observational results (Eiroa+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors &amp; temperatures of PMS stars (Pecaut+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/25">J/ApJS/211/25 : Spitzer/IRS debris disk catalog. 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