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<ri:Resource created="2019-06-05T09:40:39Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Massive SFR beyond the solar circle</title><shortName>J/MNRAS/487/1057</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/487/1057</identifier><altIdentifier>doi:10.26093/cds/vizier.74871057</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Djordjevic J.O.</name></creator><creator><name>Thompson M.A.</name></creator><creator><name>Uruqhart J.S.</name></creator><creator><name>Forbrich J.</name></creator><date role="Updated">2024-08-19T20:18:45Z</date><date role="Created">2019-06-05T09:40:39Z</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>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>We have compiled the most complete compact and ultracompact HII region catalogue to date via multi-wavelength inspection of survey data. We utilise data from the recently available SASSy 850um survey to identify massive star forming clumps in the outer Galaxy (R_GC_&gt;8.5kpc) and cross-match with infrared and radio data of known UC HII regions from the RMS database. For the inner Galaxy sample (R_GC_&lt;8.5kpc), we adopt the compact HII regions from previous works that used similar methods to cross match ATLASGAL with either CORNISH or RMS, depending on the location within the Galactic plane. We present a new UC HII region catalogue that more than doubles the original sample size of previous work, totalling 536 embedded HII regions and 445 host clumps. We examine the distance independent values of N_Ly_/M and L_bol_/M as proxies for massive star formation efficiency and overall star formation efficiency, respectively. We find a significant trend showing that L_bol_/M decreases with increasing RGC, suggesting that the overall star formation per unit mass is less in the outer Galaxy.</description><source format="bibcode">2019MNRAS.487.1057D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/487/1057</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/435/400">J/MNRAS/435/400 : ATLASGAL. Properties of compact HII regions (Urquhart+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/443/1555">J/MNRAS/443/1555 : ATLASGAL massive star forming clumps sample (Urquhart+ 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/473/1059">J/MNRAS/473/1059 : Galactic clump properties complete sample (Urquhart+, 2018)</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/MNRAS/487/1057</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/487/1057</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/487/1057</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/487/1057</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/487/1057</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/487/1057</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Millimeter</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/487/1057/table1</name><description>Derived clump properties of the host molecular clumps</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>Prop</name><description>indicates derived HII region propertie in table 2</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Submm</name><description>Submillimetre name (AGAL for ATLASGAL objects; JCMTLSY for SASSy)`</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="27*">char</dataType><flag>primary</flag></column><column><name>r_Submm</name><description>[1/3] Reference for Submm name (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Complex</name><description>? Complex that clump belongs to (if any)</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>HII</name><description>[1/13]? HII Region Density</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>vlsr</name><description>? LSR radial velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>D</name><description>? Heliocentric distance</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rgal</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>r_D</name><description>[1/4]? Reference for D (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Radius</name><description>? Effective Radius of clump</description><unit>pc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FsubmmP</name><description>Peak submillimetre flux</description><unit>Jy/beam</unit><ucd>phot.flux.density;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FsubmmInt</name><description>Integrated submillimetre flux</description><unit>Jy</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rc</name><description>? Gas-to-dust ratio value with Giannetti et al. (2015A&amp;A...580L...7G) correction</description><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LogNH2</name><description>Column density</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LogNH2c</name><description>? Corrected column density</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LogMcl</name><description>? Clump mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LogMclc</name><description>? Corrected clump mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/487/1057/table2</name><description>Derived HII region properties for a selection of the full sample</description><column><name>LogNly/M</name><description>? Lyman continuum to mass ratio</description><unit>log(ph.s**-1.solMass**-1)</unit><ucd>phys.mass;spect.continuum;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</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>Radio</name><description>Radio name (in galactic coordinates)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>r_Radio</name><description>[1/3] Reference for Radio name (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Submm</name><description>Submillimetre name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="27*">char</dataType></column><column><name>Offset</name><description>? Offset between radio and submillimetre centres</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FRadioP</name><description>? Radio peak flux</description><unit>mJy/beam</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FradioInt</name><description>? Integrated flux</description><unit>mJy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Diam</name><description>? Angular diameter</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Diampc</name><description>? Physical diameter</description><unit>pc</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Freq</name><description>? Frequency of observations</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LogNly</name><description>? Lyman continuum flux</description><unit>ph/s</unit><ucd>phot.flux;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LogLbol</name><description>? Bolometric luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LogLbol/M</name><description>? Bolomatric luminosity to mass ratio</description><unit>log(solLum.solMass**-1)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LogLbol/Mc</name><description>? 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