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<ri:Resource created="2013-08-22T14:01:37Z" 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>Disk-bearing stars in Cygnus OB2</title><shortName>J/ApJ/773/135</shortName><identifier>ivo://CDS.VizieR/J/ApJ/773/135</identifier><altIdentifier>doi:10.26093/cds/vizier.17730135</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Guarcello M.G.</name></creator><creator><name>Drake J.J.</name></creator><creator><name>Wright N.J.</name></creator><creator><name>Drew J.E.</name></creator><creator><name>Gutermuth R.A.,Hora J.L.</name></creator><creator><name>Naylor T.</name></creator><creator><name>Aldcroft T.</name></creator><creator><name>Fruscione A.</name></creator><creator><name>Garcia-alvarez D.,Kashyap V.L.</name></creator><creator><name>King R.</name></creator><date role="Updated">2014-12-16T11:15:31Z</date><date role="Created">2013-08-22T14:01:37Z</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-associations</subject><subject>pre-main-sequence-stars</subject><subject>photometry</subject><description>The formation of stars in massive clusters is one of the main modes of the star formation process. However, the study of massive star-forming regions is hampered by their typically large distances to the Sun. One exception to this is the massive star-forming region Cygnus OB2 in the Cygnus X region, at the distance of ~1400pc. Cygnus OB2 hosts very rich populations of massive and low-mass stars, being the best target in our Galaxy to study the formation of stars, circumstellar disks, and planets in the presence of massive stars. In this paper, we combine a wide and deep set of photometric data, from the r band to 24{mu}m, in order to select the disk-bearing population of stars in Cygnus OB2 and identify the class I, class II, and stars with transition and pre-transition disks. We selected 1843 sources with infrared excesses in an area of 1{deg}x1{deg} centered on Cyg OB2 in several evolutionary stages: 8.4% class I, 13.1% flat-spectrum sources, 72.9% class II, 2.3% pre-transition disks, and 3.3% transition disks. The spatial distribution of these sources shows a central cluster surrounded by an annular overdensity and some clumps of recent star formation in the outer region. Several candidate subclusters are identified, both along the overdensity and in the rest of the association.</description><source format="bibcode">2013ApJ...773..135G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/773/135</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/II/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/321">II/321 : IPHAS DR2 Source Catalogue (Barentsen+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/643/238">J/ApJ/643/238 : Chandra/2MASS sources in Cygnus OB2 (Butt+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/464/211">J/A+A/464/211 : Cyg OB2 Chandra and near-IR obs (Albacete Colombo+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/472/557">J/A+A/472/557 : Cygnus OB2 region 610MHz sources (Marti+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/384/1277">J/MNRAS/384/1277 : H{alpha} emission line sources from IPHAS (Witham+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/453">J/A+A/486/453 : Early-type stars in Cyg OB2 NIR photometry (Comeron+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/84">J/ApJS/184/84 : X-ray sources in Cyg OB2 region (Wright+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/713/871">J/ApJ/713/871 : X-ray sources in star-forming region Cyg-OB2 (Wright+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/679">J/ApJ/720/679 : Optical spectroscopy in Cygnus X region (Beerer+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/27">J/ApJS/194/27 : Variable stars in Cygnus OB2 (Henderson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/543/A101">J/A+A/543/A101 : OB stars in Cygnus OB2 association (Comeron+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/202/19">J/ApJS/202/19 : GTC/OSIRIS riz photometry in Cyg OB2 (Guarcello+, 2012)</relatedResource><relatedResource>http://www.iphas.org/ : IPHAS Home Page</relatedResource><relatedResource>http://www.sdss.org/ : SDSS Home Page</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Spitzer/IRAC 8.0um magnitude</description><unit>mag</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[8.0]</name><description>? rms uncertainty on [8.0]</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[24]</name><description>? 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(2009ApJS..184...18G) method</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S2</name><description>[0/1] 1 if the star has been selected with the [4.5] versus [4.5]-[8.0] diagram</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S3</name><description>[0/1] 1 if the star has been selected with the [3.6] versus [3.6]-[24] diagram</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S4</name><description>[0/1] 1 if the star has been selected with the [24] versus [8.0]-[24] diagram</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S5</name><description>[0/1] 1 if the star has been selected with the [4.5]-[5.8] versus [5.8]-[24] diagram</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S6</name><description>[0/1] 1 if the star has been selected with the [24] versus [4.5]-[8.0] diagram</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S7</name><description>[0/1] 1 if the star has been selected with the QriJ[3.6] index (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S8</name><description>[0/1] 1 if the star has been selected with the QriJ[4.5] index (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S9</name><description>[0/1] 1 if the star has been selected with the QriJ[5.8] index (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S10</name><description>[0/1] 1 if the star has been selected with the QriJ[8.0] index (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S11</name><description>[0/1] 1 if the star has been selected with the J-H versus H-K diagram</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S12</name><description>[0/1] 1 if the star has been selected with the QJHHK index (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S13</name><description>[0/1] 1 if the star has been selected with the QriHK index (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nS</name><description>[1/13] Number of positive selection criteria ({Sigma}S_i_)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>alpha</name><description>? Infrared spectral index {alpha} = dlog({lambda}F_{lambda}_)/dlog({lambda}).</description><ucd>spect.index;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Class</name><description>Classification (2)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column></table></schema></tableset></ri:Resource>