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<ri:Resource created="2021-08-20T13:15:08Z" status="active" updated="2025-06-13T15:25:00Z" 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>Young stellar objects in W49A and W51</title><shortName>J/MNRAS/477/3369</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/477/3369</identifier><altIdentifier>doi:10.26093/cds/vizier.74773369</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Eden D.J.</name></creator><creator><name>Moore T.J.T.</name></creator><creator><name>Urquhart J.S.</name></creator><creator><name>Elia D.</name></creator><creator><name>Plume R.</name></creator><creator><name>Konig C.,Baldeschi A.</name></creator><creator><name>Schisano E.</name></creator><creator><name>Rigby A.J.</name></creator><creator><name>Morgan L.K.</name></creator><creator><name>Thompson M.A.</name></creator><date role="Updated">2024-08-18T20:19:13Z</date><date role="Created">2021-08-20T13:15:08Z</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>star-forming-regions</subject><subject>young-stellar-objects</subject><subject>galaxy-classification-systems</subject><description>We have compared the star-formation properties of the W49A and W51 regions by using far-infrared data from the Herschel infrared Galactic Plane Survey (Hi-GAL) and 850-um observations from the James Clerk Maxwell Telescope (JCMT) to obtain luminosities and masses, respectively, of associated compact sources. The former are infrared luminosities from the catalogue of Elia et al., while the latter are from the JCMT Plane survey source catalogue as well as measurements from new data. The clump-mass distributions of the two regions are found to be consistent with each other, as are the clump-formation efficiency and star-formation efficiency analogues. However, the frequency distributions of the luminosities of the young stellar objects are significantly different. While the luminosity distribution in W51 is consistent with Galaxy-wide samples, that of W49A is top heavy. The differences are not dramatic and are concentrated in the central regions of W49A. However, they suggest that physical conditions there, which are comparable in part to those in extragalactic starbursts, are significantly affecting the star-formation properties or evolution of the dense clumps in the region.</description><source format="bibcode">2018MNRAS.477.3369E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/477/3369</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/MNRAS/469/2163">J/MNRAS/469/2163 : JCMT Plane Survey. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>W49A Source Catalogue Name (W49_NNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>GLON</name><description>Galactic longitude of peak position</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude of peak position</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>GLONc</name><description>Galactic longitude of central position</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLATc</name><description>Galactic latitude of central position</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>amaj</name><description>Semi-major axis</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>bmin</name><description>Semi-minor axis</description><unit>arcsec</unit><ucd>phys.angSize.sminAxis</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PA</name><description>Position angle of source</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Reff</name><description>Effective radius of the source</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Fpeak</name><description>Peak flux at 850um</description><unit>Jy/beam</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Fpeak</name><description>Error on the peak flux</description><unit>Jy/beam</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fint</name><description>Integrated flux at 850um</description><unit>Jy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SNR</name><description>Signal-to-noise ratio</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Fint</name><description>Error on the integrated flux</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W49Aflag</name><description>[y/n] Flag if the source is associated with W49A</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/MNRAS/477/3369/tableb1</name><description>The JPS sources associated with the W51 star-forming region</description><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. 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