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<ri:Resource created="2006-01-12T09:02:16Z" status="active" updated="2026-03-17T20:04:00Z" 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>Molecular clouds in southern HII regions</title><shortName>J/PASJ/51/791</shortName><identifier>ivo://CDS.VizieR/J/PASJ/51/791</identifier><altIdentifier>doi:10.26093/cds/vizier/bj-1k-rq</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yamaguchi R.</name></creator><creator><name>Saito H.</name></creator><creator><name>Mizuno N.</name></creator><creator><name>Mine Y.</name></creator><creator><name>Mizuno A.</name></creator><creator><name>Ogawa H.</name></creator><creator><name>Fukui Y.</name></creator><date role="Updated">2026-03-17T20:04:00Z</date><date role="Created">2006-01-12T09:02:16Z</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>molecular-clouds</subject><subject>infrared-sources</subject><description>We have carried out extensive ^13^CO(J=1-0) observations toward 23 southern H II regions associated with bright-rimmed clouds. In total, 95 molecular clouds have been identified to be associated with the H II regions. Among the 95, 57 clouds are found to be associated with 204 IRAS point sources which are candidates for young stellar objects. There is a significant increase of star-formation efficiency on the side facing to the H II regions; the luminosity-to-mass ratio, defined as the ratio of the stellar luminosity to the molecular cloud mass, is higher by an order of magnitude on the near side of the H II regions than that on the. far side. This indicates that molecular gas facing to the H II regions is more actively forming massive stars whose luminosity is ~&gt;10^3^L_{sun}_. In addition, the number density of the IRAS point sources increases by a factor of 2 on the near side of the H II regions compared with on the far side. These results strongly suggest that the active formation of massive stars on the near side of the H II regions is due to the effects of the H II regions, such as the compression of molecular material by the ionization/shock fronts. For the whole Galaxy, we estimate that the present star-formation rate under such effects is at least 0.2-0.4M_{sun}_/yr, corresponding to a few 10% by mass.</description><source format="bibcode">1999PASJ...51..791Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/51/791</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/VII/20">VII/20 : Catalogue of HII Regions (Sharpless 1959)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/284/233">J/A+A/284/233 : Association of HII regions &amp; IRAS PSC sources (Codella+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/133/29">J/A+AS/133/29 : Molecular line survey towards UC HII (Hatchell+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/131/319">J/A+AS/131/319 : HII regions catalogue (Petit+ 1998)</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/PASJ/51/791</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASJ/51/791</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASJ/51/791</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASJ/51/791</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/PASJ/51/791</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASJ/51/791</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/PASJ/51/791/clouds (Properties of ^13^CO clouds)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASJ/51/791/clouds?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/PASJ/51/791/clouds?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASJ/51/791/clouds?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>112.738845</ra><dec>-18.930261</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/9820 10628 6/20805 21504 28817 28819 28888 28890-28892 28894 37817 37819 37850-37851 37872 37891 37894 37896-37897 37932 37938 39133 39163 39257-39259 39329 39331 39398 40618-40619 41598-41599 41661 41696 41698 41813 42187 42190 42212-42213 42407 42516 42518 42520</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/PASJ/51/791?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/PASJ/51/791/table1</name><description>Observed H II regions</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>HII</name><description>HII region</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType><flag>primary</flag></column><column><name>Size</name><description>Size (NN or NNNxNNN) in arcmin (1)</description><unit>arcmin</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Star</name><description>Exciting star</description><ucd>meta.id.assoc</ucd></column><column><name>n_Star</name><description>[+] +: the earliest star probably contributing to ionization</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SpType</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Dist</name><description>? 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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>Ref</name><description>Reference number</description><ucd>meta.id;meta.main</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="20*">char</dataType></column><column><name>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column></table><table><name>J/PASJ/51/791/clouds</name><description>Properties of ^13^CO clouds</description><column><name>tau</name><description>? Optical depth</description><ucd>phys.absorption.opticalDepth</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>[YSM99]</name><description>[1-95] Sequential number</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>Cloud</name><description>Cloud name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">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><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RA1950</name><description>Right ascension (1950)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE1950</name><description>Declination (1950)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>TR*</name><description>Peak antenna temperature (1)</description><unit>K</unit><ucd>phot.antennaTemp</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DV</name><description>FWHM line width (1)</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vlsr</name><description>LSR velocity (1)</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Int</name><description>Velocity-integrated intensity (1)</description><unit>K.km/s</unit><ucd>phot.flux.density;em.mm.100-200GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N(H2)</name><description>H_2_ column density</description><unit>1e+21cm**-2</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DVc</name><description>? FWHM line width computed from gaussian fit</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>? Distance to the molecular cloud</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rad</name><description>? Size of the molecular cloud</description><unit>pc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mass</name><description>? 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