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<ri:Resource created="2012-09-10T12:24:18Z" 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>Intermediate-mass stars in IC 1805</title><shortName>J/ApJ/726/19</shortName><identifier>ivo://CDS.VizieR/J/ApJ/726/19</identifier><altIdentifier>doi:10.26093/cds/vizier.17260019</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wolff S.C.</name></creator><creator><name>Strom S.E.</name></creator><creator><name>Rebull L.M.</name></creator><date role="Updated">2017-12-05T05:10:21Z</date><date role="Created">2012-09-10T12:24:18Z</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>open-star-clusters</subject><subject>stellar-spectral-types</subject><subject>line-intensities</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>interstellar-reddening</subject><subject>young-stellar-objects</subject><description>We report the results of a study of the intermediate- and high-mass stars in the young, rich star-forming complex IC 1805, based on a combination of optical, near-infrared, and mid-infrared photometry, and classification spectra. These data provide the basis for characterizing the masses and ages for stars more massive than ~2M_{sun}_ and enable a study of the frequency and character of circumstellar disks associated with intermediate- and high-mass stars. Optically thick accretion disks among stars with masses 2&lt;M/M_{sun}_&lt;4 are rare (~2% of members) and absent among more massive stars. A larger fraction (~10%) of stars with masses 2&lt;M/M_{sun}_&lt;4 appear to be surrounded by disks that have evolved from the initial optically thick accretion phase. We identify four classes of such disks. These classes are based on spectral energy distributions (SEDs) of excess emission above photospheric levels: disks that are (1) optically thin based on the magnitude of the observed excess emission from 2 to 24um, (2) optically thin in their inner regions (r&lt;20AU) and optically thick in their outer regions, (3) exhibit empty inner regions (r&lt;10AU) and optically thin emission in their outer regions, and (4) exhibit empty inner regions and optically thick outer regions. We discuss, and assess the merits and liabilities of, proposed explanations for disks exhibiting these SED types and suggest additional observations that would test these proposals.</description><source format="bibcode">2011ApJ...726...19W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/726/19</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/96">V/96 : Catalogue of open cluster parameters from UBV-data. (Loktin+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/726/18">J/ApJ/726/18 : Disk evolution in W5: stars at 2-5Myr (Koenig+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/462">J/AJ/140/462 : Intermediate-mass star-forming regions (Arvidsson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/407/2109">J/MNRAS/407/2109 : Kinematic study of open clusters (Vande Putte+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/172">J/ApJS/184/172 : High- and intermediate-mass YSOs in the LMC (Gruendl+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/179/451">J/ApJS/179/451 : IR excesses for protoplanetary disks (Kenyon+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1092">J/AJ/133/1092 : vsini of B0-B3 stars in 7 young clusters (Wolff+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/382/1073">J/MNRAS/382/1073 : M/L relation of intermediate-mass stars (Malkov+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/464/581">J/A+A/464/581 : Sco OB2 intermediate-mass stars (Kouwenhoven+, 2007)</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/648/591">J/ApJ/648/591 : Stellar rotation in young clusters. 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