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<ri:Resource created="2013-03-19T15:43:53Z" 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>Distances of 793 BGPS sources</title><shortName>J/MNRAS/422/3178</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/422/3178</identifier><altIdentifier>doi:10.26093/cds/vizier.74223178</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>Plume R.</name></creator><creator><name>Morgan L.K.</name></creator><date role="Updated">2024-07-17T20:15:47Z</date><date role="Created">2013-03-19T15:43:53Z</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>molecular-clouds</subject><subject>stellar-distance</subject><subject>radial-velocity</subject><description>By positional matching to the catalogue of Galactic Ring Survey molecular clouds, we have derived distances to 793 Bolocam Galactic Plane Survey (BGPS) sources out of a possible 806 located within the region defined by Galactic longitudes l=28.5{deg}-31.5{deg} and latitudes |b|&lt;=1{deg}. This section of the Galactic plane contains several major features of Galactic structure at different distances, mainly mid-arm sections of the Perseus and Sagittarius spiral arms and the tangent of the Scutum-Centaurus arm, which is coincident with the end of the Galactic long bar. By utilizing the catalogued cloud distances plus new kinematic distance determinations, we are able to separate the dense BGPS clumps into these three main line-of-sight components to look for variations in star formation properties that might be related to the different Galactic environments. We find no evidence of any difference in either the clump mass function or the average clump formation efficiency (CFE) between these components that might be attributed to environmental effects on scales comparable to Galactic structure features.</description><source format="bibcode">2012MNRAS.422.3178E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/422/3178</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/ApJ/699/1153">J/ApJ/699/1153 : GRS molecular clouds kinematic distances (Roman-Duval+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/131">J/ApJS/182/131 : Molecular clouds and clumps in the GRS (Rathborne+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/492">J/ApJ/723/492 : GRS molecular clouds physical properties (Roman-Duval+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/721/137">J/ApJ/721/137 : Bolocam Galactic Plane Survey (BGPS) (Bally+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/123">J/ApJS/188/123 : Bolocam Galactic Plane Survey (BGPS). II. (Rosolowsky+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/195/14">J/ApJS/195/14 : Bolocam Galactic Plane Survey (BGPS). V. 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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>GRS</name><description>GRS cloud name (GLLL.ll+BB.bb)</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Vlsr</name><description>GRS cloud LSR velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>? GRS cloud Distance</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BGPS</name><description>[3984/4789] BGPS source number (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GLON</name><description>BGPS source Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>BGPS source Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/MNRAS/422/3178/table2</name><description>Summary of unassociated BGPS sources and their derived kinematic distances</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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