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<ri:Resource created="2019-08-12T10:38:44Z" 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>Ionization profiles of 8 Galactic H II regions</title><shortName>J/ApJS/241/2</shortName><identifier>ivo://CDS.VizieR/J/ApJS/241/2</identifier><altIdentifier>doi:10.26093/cds/vizier.22410002</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Luisi M.</name></creator><creator><name>Anderson L.D.</name></creator><creator><name>Liu B.</name></creator><creator><name>Roshi D.A.</name></creator><creator><name>Churchwell Ed</name></creator><date role="Updated">2019-08-21T06:52:30Z</date><date role="Created">2019-08-12T10:38:44Z</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>interstellar-medium</subject><subject>radio-astronomy</subject><description>Using Green Bank Telescope radio recombination line (RRL) data, we analyze the role of leaking radiation from HII regions in maintaining the ionization of the interstellar medium (ISM). We observed a sample of eight Galactic HII regions of various sizes, morphologies, and luminosities. For each region, the hydrogen RRL intensity decreases roughly as a power-law with the distance from the center of the region. This suggests that radiation leaking from the HII region is responsible for the majority of surrounding ionized gas producing RRL emission. Our results further indicate that the hydrogen RRL intensity appears to be fundamentally related to the HII region sizes traced by their photodissociation regions, such that physically smaller HII regions show a steeper decrease in intensity with an increasing distance from the region centers. As a result, giant HII regions may have a much larger effect in maintaining the ionization of the ISM. For six of the eight observed HII regions, we find a decrease in the ^4^He^+^/H^+^ abundance ratio with an increasing distance, indicating that He-ionizing photons are being absorbed within the ionization front of the HII region. There is enhanced carbon RRL emission toward directions with strong continuum background, suggesting that the carbon emission is amplified by stimulated emission.</description><source format="bibcode">2019ApJS..241....2L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/241/2</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/III/274">III/274 : Galactic O-Star Spectroscopic Survey (GOSSS) (Sota+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/653/1226">J/ApJ/653/1226 : Physical properties of galactic HII regions (Quireza+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/169/353">J/ApJS/169/353 : Chandra sources in M17 (Broos+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/738/27">J/ApJ/738/27 : Galactic HII regions RRL and continuum data (Balser+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/411/705">J/MNRAS/411/705 : Spectrophotometric distances of HII regions (Moises+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/755/40">J/ApJ/755/40 : HII reg. in Magellanic clouds from MCELS (Pellegrini+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/34">J/ApJ/764/34 : HRDS IV. H, He &amp; C radio recombination lines (Wenger+, 2013)</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/810/42">J/ApJ/810/42 : Hydrogen RRL parameters of H II regions (Anderson+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/240/14">J/ApJS/240/14 : SIGGMA: inner galaxy data release (Liu+, 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/241/2</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/241/2</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/241/2</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/241/2</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/241/2</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/241/2</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/241/2/table1 (H II region properties)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/241/2/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/241/2/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/241/2/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>275.18216</ra><dec>-16.16153</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJS/241/2/pointings (Observed positions (table 3) and radio continuum temperatures and source properties (table 5))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/241/2/pointings?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/241/2/pointings?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/241/2/pointings?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>60.815833</ra><dec>51.315</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1781 1783 14641 21438 21439 29113 29116 29118 29119 29463 29469 29504 30256 30259 30262 30622 30644</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/241/2?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/241/2/table1</name><description>H II region properties</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></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>Reg</name><description>HII region identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType><flag>primary</flag></column><column><name>OName</name><description>Other name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">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>Rad</name><description>[2.4/14.2] Radius of the HII region (see Section 3)</description><unit>pc</unit><ucd>phys.size.radius;obs.field</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rgal</name><description>[4.5/11.6] Galactocentric radius</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[0.4/8.4] Distance to the Sun from Anderson+, 2014, J/ApJS/212/1</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpT</name><description>Spectral type of the ionizing source(s)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>r_SpT</name><description>[1/8] Reference (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Np</name><description>Number of pointings in this region (link to Tables 3+5)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</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. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/ApJS/241/2/pointings</name><description>Observed positions (table 3) and radio continuum temperatures and source properties (table 5)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Emission measure</description><unit>pc.cm**-6</unit><ucd>phys.emissMeasure</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_EM</name><description>[360/492550]? 1{sigma} uncertainty in EM</description><unit>pc.cm**-6</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/ApJS/241/2/table4</name><description>H, He, and C RRL parameters for the 98 sources</description><column><name>Reg</name><description>HII region identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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