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<ri:Resource created="2007-10-27T16:21:04Z" 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>H II absorption regions at 74MHz</title><shortName>J/AJ/132/242</shortName><identifier>ivo://CDS.VizieR/J/AJ/132/242</identifier><altIdentifier>doi:10.26093/cds/vizier.51320242</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nord M.E.</name></creator><creator><name>Henning P.A.</name></creator><creator><name>Rand R.J.</name></creator><creator><name>Lazio T.J.W.</name></creator><creator><name>Kassim N.E.</name></creator><date role="Updated">2019-03-05T10:48:01Z</date><date role="Created">2007-10-27T16:21:04Z</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>effective-temperature</subject><description>In this work we present 74MHz observations in the region 26{deg}&gt;l&gt;-15{deg}, -5{deg}&lt;b&lt;5{deg} report the detection of 92 absorption features associated with known HII regions; and derive the brightness temperature of the Galactic cosmic-ray electron synchrotron emission emanating from the column behind these regions. For the 42 HII regions with known distances, the average emissivity of the column behind the HII region is derived. The 74MHz emissivity values range between 0.3 and 1.0K/pc for a model assuming uniform distribution of emissivity. Methods for using this type of data to model the three-dimensional distribution of cosmic-ray emissivity and the possibility of using this method to break the HII region kinematic distance degeneracy are discussed.</description><source format="bibcode">2006AJ....132..242N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/132/242</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+AS/131/319">J/A+AS/131/319 : HII regions catalogue (Petit+ 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