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<ri:Resource created="2022-03-04T14:08:09Z" status="active" updated="2025-11-05T20:18:45Z" 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>High-mass star formation evolutionary trends</title><shortName>J/MNRAS/510/3389</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/510/3389</identifier><altIdentifier>doi:10.26093/cds/vizier.75103389</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Urquhart J.S.</name></creator><creator><name>Wells M.R.A.</name></creator><creator><name>Pillai T.</name></creator><creator><name>Leurini S.</name></creator><creator><name>Giannetti A.,Moore T.J.T.</name></creator><creator><name>Thompson M.A.</name></creator><creator><name>Figura C.</name></creator><creator><name>Colombo D.</name></creator><creator><name>Yang A.Y.</name></creator><creator><name>Koeonig C.,Wyrowski F.</name></creator><creator><name>Menten K.M.</name></creator><creator><name>Rigby A.J.</name></creator><creator><name>Eden D.J.</name></creator><creator><name>Ragan S.E.</name></creator><date role="Updated">2025-11-05T20:18:45Z</date><date role="Created">2022-03-04T14:08:09Z</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>star-forming-regions</subject><subject>early-type-stars</subject><subject>stellar-distance</subject><description>ATLASGAL is an 870um dust survey of 420deg^2^ the inner Galactic plane and has been used to identify ~10000 dense molecular clumps. Dedicated follow-up observations and complementary surveys are used to characterize the physical properties of these clumps, map their Galactic distribution, and investigate the evolutionary sequence for high-mass star formation. The analysis of the ATLASGAL data is ongoing: We present an up-to-date version of the catalogue. We have classified 5007 clumps into four evolutionary stages (quiescent, protostellar, young stellar objects and HII regions) and find similar numbers of clumps in each stage, suggesting a similar lifetime. The luminosity-to-mass (L_bol_/M_fwhm_) ratio curve shows a smooth distribution with no significant kinks or discontinuities when compared to the mean values for evolutionary stages indicating that the star formation process is continuous and that the observational stages do not represent fundamentally different stages or changes in the physical mechanisms involved. We compare the evolutionary sample with other star formation tracers (methanol and water masers, extended green objects and molecular outflows) and find that the association rates with these increases as a function of evolutionary stage, confirming that our classification is reliable. This also reveals a high association rate between quiescent sources and molecular outflows, revealing that outflows are the earliest indication that star formation has begun and that star formation is already ongoing in many of the clumps that are dark even at 70um.</description><source format="bibcode">2022MNRAS.510.3389U</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/510/3389</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/A+A/540/A113">J/A+A/540/A113 : Starless clumps in ATLASGAL (Tackenberg+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A146">J/A+A/544/A146 : ATLASGAL cold high-mass clumps with NH_3_ (Wienen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A45">J/A+A/549/A45 : ATLASGAL Compact Source Catalog: 330&lt;l&lt;21 (Contreras+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/1752">J/MNRAS/431/1752 : ATLASGAL 6.7GHz methanol masers (Urquhart+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/435/400">J/MNRAS/435/400 : ATLASGAL. 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analysis</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Param</name><description>indicates derived clump parameters in table6</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Clump</name><description>ATLASGAL catalogue name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType><flag>primary</flag></column><column><name>VLSR</name><description>? Radial Velocity (-999 indicates non-detection)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_VLSR</name><description>Shorthand reference for VLSR, in refs.dat file</description><ucd>meta.ref;phys.veloc;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>DReid</name><description>? Reid et al. (2019ApJ...885..131R) distance</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dnear</name><description>? Reid Near distance solution</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dfar</name><description>? 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The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Assigned heliocentric distance</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RGC</name><description>? Galactocentric distance</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RFWHM</name><description>? FWHM radius</description><unit>pc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logL</name><description>? Log of the luminosity in solar luminosities</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logMFWHM</name><description>? Log of the FWHM mass in solar masses</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NH2</name><description>? H2 volume density</description><unit>cm**-3</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tauff</name><description>? Free-fall timescale</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>L/MFWHM</name><description>? Luminosity/M_FWHM_ ratio</description><unit>solLum/solMass</unit><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/510/3389/table6</name><description>Physical parameters for the complexes identified</description><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Association catalogue name</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Complex</name><description>Literature name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="40*">char</dataType></column><column><name>NumAssoc</name><description>Number of associated clumps</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GLON</name><description>Mean longitude of associated clumps</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>e_GLON</name><description>Uncertainty in mean longitude of associated clumps</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GLAT</name><description>Mean latitude of associated clumps</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>e_GLAT</name><description>Uncertainty in mean latitude of associated clumps</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VLSR</name><description>Mean radial Velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_VLSR</name><description>Uncertainty in radial Velocity</description><unit>km/s</unit><ucd>stat.error;phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>Heliocentric distance</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RGC</name><description>Galactocentric distance</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tdust</name><description>? Dust temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Tdust</name><description>? Uncertainty in dust temperature</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logLcl</name><description>? Log of the cluster luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lclpc</name><description>? Percentage of total luminosity from sample</description><unit>%</unit><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logMclr</name><description>? Log of the cluster mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mclpc</name><description>? Percentage of total mass from sample</description><unit>%</unit><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>L/M</name><description>? Cluster Luminosity/Mass_FWHM ratio</description><unit>solLum/solMass</unit><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/510/3389/refs</name><description>References</description><column><name>Ref</name><description>Reference code</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="27*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BibCode</name><description>BibCode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Aut</name><description>Author's name</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column></table></schema></tableset></ri:Resource>