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<ri:Resource created="2017-01-12T08:46:52Z" 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>Hi-GAL cluster candidates physical properties</title><shortName>J/A+A/597/A114</shortName><identifier>ivo://CDS.VizieR/J/A+A/597/A114</identifier><altIdentifier>doi:10.26093/cds/vizier.35970114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Beuret M.</name></creator><creator><name>Billot N.</name></creator><creator><name>Cambresy L.</name></creator><creator><name>Eden D.J.</name></creator><creator><name>Elia D.</name></creator><creator><name>Molinari S.,Pezzuto S.</name></creator><creator><name>Schisano E.</name></creator><date role="Updated">2017-01-12T07:47:50Z</date><date role="Created">2017-01-12T08:46:52Z</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>milky-way-galaxy</subject><subject>interstellar-medium</subject><subject>infrared-sources</subject><subject>h-ii-regions</subject><description>The aims are to investigate the clustering of the far-infrared sources from the Herschel infrared Galactic Plane Survey (Hi-GAL) in the Galactic longitude range of -71 to 67{deg}. These clumps, and their spatial distribution, are an imprint of the original conditions within a molecular cloud. This will produce a catalogue of over-densities. The minimum spanning tree (MST) method was used to identify the over-densities in two dimensions. The catalogue was further refined by folding in heliocentric distances, resulting in more reliable over-densities, which are cluster candidates. We found 1633 over-densities with more than ten members. Of these, 496 are defined as cluster candidates because of the reliability of the distances, with a further 1,137 potential cluster candidates. The spatial distributions of the cluster candidates are different in the first and fourth quadrants, with all clusters following the spiral structure of the Milky Way. The cluster candidates are fractal. The clump mass functions of the clustered and isolated are statistically indistinguishable from each other and are consistent with Kroupa's initial mass function.</description><source format="bibcode">2017A&amp;A...597A.114B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/597/A114</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/397/213">J/A+A/397/213 : Galactic HII regions (Paladini+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/212/1">J/ApJS/212/1 : The WISE catalog of Galactic HII regions (Anderson+, 2014)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/597/A114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/597/A114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/597/A114</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/597/A114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/597/A114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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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>Cluster candidate name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>GLON</name><description>Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>amaj</name><description>Major axis</description><unit>arcmin</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>bmin</name><description>Minor axis</description><unit>arcmin</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA</name><description>Position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dpeak</name><description>Heliocentric distance estimated from the peak of the heliocentric distance estimates histogram of the clumps</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dmean</name><description>Mean of the heliocentric distance estimates of the clumps</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dgal</name><description>Galactocentric distance (1)</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Z</name><description>Scale height (2)</description><unit>pc</unit><ucd>pos.cartesian.z;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lamaj</name><description>Linear major axis (2)</description><unit>pc</unit><ucd>phys.size</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lbmin</name><description>Linear minor axis (2)</description><unit>pc</unit><ucd>phys.size</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dens</name><description>Surface density</description><unit>pc**-2</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nclumps</name><description>Number of clumps</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Rclumps</name><description>? Ratio of the number of pre-stellar clumps over proto-stellar clumps</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_Rclumps</name><description>[ab] Note when no value (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>HII</name><description>Closest HII region (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Flag</name><description>[1,2]? 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