<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2021-05-06T16:14:08Z" 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>VLA 9GHz obs. of HII region candidates</title><shortName>J/ApJS/253/23</shortName><identifier>ivo://CDS.VizieR/J/ApJS/253/23</identifier><altIdentifier>doi:10.26093/cds/vizier.22530023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Armentrout W.P.</name></creator><creator><name>Anderson L.D.</name></creator><creator><name>Wenger T.V.</name></creator><creator><name>Balser D.S.</name></creator><creator><name>Bania T.M.</name></creator><date role="Updated">2023-08-16T14:19:32Z</date><date role="Created">2021-05-06T16:14:08Z</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>radio-continuum-emission</subject><subject>infrared-sources</subject><description>The Milky Way contains thousands of HII region candidates identified by their characteristic mid-infrared morphology, but lacking detections of ionized gas tracers such as radio continuum or radio recombination line emission. These targets thus remain unconfirmed as HII regions. With only ~2500 confirmed HII regions in the Milky Way, Galactic surveys are deficient by several thousand nebulae when compared to external galaxies with similar star formation rates. Using sensitive 9 GHz radio continuum observations with the Karl G. Jansky Very Large Array, we explore a sample of HII region candidates in order to set observational limits on the actual total population of Galactic HII regions. We target all infrared-identified "radio-quiet" sources from the Wide-field Infrared Survey Explorer Catalog of Galactic HII regions between 245{deg}&gt;=l&gt;=90{deg} with infrared diameters less than 80". We detect radio continuum emission from 50% of the targeted HII region candidates, providing strong evidence that most of the radio-quiet candidates are bona fide HII regions. We measure the peak and integrated radio flux densities and compare the inferred Lyman continuum fluxes using models of OB stars. We conclude that stars of approximately spectral type B2 and earlier are able to create HII regions with similar infrared and radio continuum morphologies as the more luminous HII regions created by O stars. From our 50% detection rate of "radio-quiet" sources, we set a lower limit of ~7000 for the HII region population of the Galaxy. Thus the vast majority of the Milky Way's HII regions remain to be discovered.</description><source format="bibcode">2021ApJS..253...23A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/253/23</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/VIII/58">VIII/58 : A Survey of Radio H II Regions in the Northern Sky (Lockman+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/171/261">J/A+A/171/261 : RRLs of Southern HII Regions (Caswell+ 1987)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1632">J/AJ/127/1632 : UBVR(UIT) photometry of O and OB stars in SMC (Oey+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/32">J/ApJS/194/32 : The HII Region Discovery Survey (HRDS). II. (Anderson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/1925">J/MNRAS/424/1925 : Spectrocopic Binarity of O and B type stars (Chini+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/2442">J/MNRAS/424/2442 : Catalog of bubbles from Milky Way Project (Simpson+, 2012)</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><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/784/111">J/ApJ/784/111 : Morphology of cand. intermediate-mass SFRs (Lundquist+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/221/26">J/ApJS/221/26 : Radio obs. of Galactic WISE HII regions (Anderson+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/199">J/ApJ/806/199 : RRL &amp; continuum data of 21 Gal. H II regions (Balser+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/799/153">J/ApJ/799/153 : Yellowballs in Milky Way project (Kerton+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/588/A97">J/A+A/588/A97 : Continuum sources from the THOR survey (Bihr+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/234/33">J/ApJS/234/33 : A GBT survey of large Galactic HII regions (Anderson+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/870/32">J/ApJ/870/32 : Kinematics in young star clusters &amp; associations (Kuhn+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/627/A175">J/A+A/627/A175 : GLOSTAR. Radio Source Catalogue I (Medina+ 2019)</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/ApJS/253/23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/253/23</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/253/23</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/253/23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/253/23</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/253/23</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/ApJS/253/23/tablea1 (*VLA radio continuum parameters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/253/23/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/253/23/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/253/23/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>316.0826667</ra><dec>49.7483611</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1307-1308 1329 1354 1433 1481 1791 1808 1848 1930 1962-1963 3031 3063 3157 3175 3302 3329 3342 3606 3609 3637-3639 3641 3644 3649 3728 3748 14263 14267 14270 14299 14306-14308 14316-14317 14321 14335 15390-15391 15409 15414 15434-15435 15438 15448-15449 15451 15456 15458 15460-15461 15469 15472 15474-15476 15621 15623-15624 15626 15629 15649 15676 15759 21457 21504 21510 21542 21671 22038 22045 22122 22208 22220 23637 23674 23765 23767 23773 23938 23968-23969 23982 24325 24426 24493 24507 24554 39804 39926 39935 40619</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/253/23?format=ascii</footprint><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/253/23/tablea1</name><description>*VLA radio continuum parameters</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>WISE</name><description>WISE identifier (GLLL.lll+BB.bbb) from Anderson+, 2014, J/ApJS/212/1 (&lt;[ABB2014] WISE GLLL.ll+BB.bbb&gt; in Simbad)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Sint</name><description>[0.12/164.1]? Integrated flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.6-12GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Sint</name><description>[0.02/17.1]? Uncertainty in Sint</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Speak</name><description>[0.014/8]? peak flux density</description><unit>mJy/beam</unit><ucd>phot.flux.density;em.radio.6-12GHz;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Speak</name><description>[0.003/2.4] Uncertainty (map RMS) for Speak (1)</description><unit>mJy/beam</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Area</name><description>[370/27270]? Region area (2)</description><unit>arcsec**2</unit><ucd>phys.area;obs.field</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Exp</name><description>[4/16] Integration time</description><unit>min</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Fig4</name><description>Figure sub-number on Figure 4 (column added by the author) (3)</description><ucd>meta.bib.fig</ucd><dataType xsi:type="vs:VOTableType">int</dataType></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></schema></tableset></ri:Resource>