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<ri:Resource created="2014-02-14T08:32:37Z" 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>YSOs from SED fitting in six HII regions</title><shortName>J/AJ/144/173</shortName><identifier>ivo://CDS.VizieR/J/AJ/144/173</identifier><altIdentifier>doi:10.26093/cds/vizier.51440173</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dirienzo W.J.</name></creator><creator><name>Indebetouw R.</name></creator><creator><name>Brogan C.</name></creator><creator><name>Cyganowski C.J.</name></creator><creator><name>Churchwell E.,Friesen R.K.</name></creator><date role="Updated">2019-12-03T10:56:19Z</date><date role="Created">2014-02-14T08:32:37Z</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>h-ii-regions</subject><subject>young-stellar-objects</subject><subject>stellar-masses</subject><subject>radial-velocity</subject><subject>galaxy-kinematics</subject><description>We investigated six HII regions with infrared, bright rimmed bubble or cometary morphology, in search of quantitative evidence for triggered star formation, both collect and collapse and radiatively driven implosion (RDI). We identified and classified 458 young stellar objects (YSOs) in and around the HII regions. YSOs were determined by fitting a collection of radiative transfer model spectral energy distributions to infrared photometry for a large sample of point sources. We determined areas where there exist enhanced populations of relatively unevolved YSOs on the bright rims of these regions, suggesting that star formation has been triggered there. We further investigated the physical properties of the regions by using radio continuum emission as a proxy for ionizing flux powering the HII regions, and ^13^CO(1-0) observations to measure masses and gravitational stability of molecular clumps. We used an analytical model of collect and collapse triggered star formation, as well as a simulation of RDI, and thus we compare the observed properties of the molecular gas with those predicted in the triggering scenarios. Notably, those regions in our sample that show evidence of cometary, or "blister", morphology are more likely to show evidence of triggering.</description><source format="bibcode">2012AJ....144..173D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/144/173</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/293">II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)</relatedResource><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/VIII/58">VIII/58 : A Survey of Radio H II Regions in the Northern Sky (Lockman+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/2442">J/MNRAS/424/2442 : Catalog of bubbles from Milky Way Project (Simpson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/741/110">J/ApJ/741/110 : The BGPS. 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