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<ri:Resource created="2021-05-05T07:44:41Z" status="active" updated="2026-03-17T20:05:49Z" 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>FUGIN. VII. Galactic plane HI clouds</title><shortName>J/PASJ/72/43</shortName><identifier>ivo://CDS.VizieR/J/PASJ/72/43</identifier><altIdentifier>doi:10.26093/cds/vizier/bj-28-1b</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nakanishi H.</name></creator><creator><name>Fujita S.</name></creator><creator><name>Tachihara K.</name></creator><creator><name>et AL.</name></creator><date role="Updated">2026-03-17T20:05:49Z</date><date role="Created">2021-05-05T07:44:41Z</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>galaxy-planes</subject><subject>milky-way-galaxy</subject><subject>molecular-clouds</subject><subject>h-i-line-emission</subject><subject>galaxy-kinematics</subject><description>We analyze molecular-gas formation in neutral atomic hydrogen (HI) clouds using the latest CO data, obtained from the FOREST (four-beam receiver system on the 45m telescope) unbiased Galactic plane imaging survey with the Nobeyama 45m telescope, and using HI data taken from the Very Large Array Galactic plane survey. We applied a dendrogram algorithm to the HI data cube to identify HI clouds, and we calculated the HI mass and molecular-gas mass by summing the CO line intensity within each HI cloud. On the basis of the results, we created a catalog of 5737 identified HI clouds with local standard of rest (LSR) velocity of VLSR&lt;=-20km/s in galactic longitude and latitude ranges of 20{deg}&lt;=l&lt;=50{deg} and -1{deg}&lt;=b&lt;=1{deg}, respectively. We found that most of the HI clouds are distributed within a Galactocentric distance of 16kpc, and most of them are in the cold neutral medium phase. In addition, we determined that the high-mass end of the HI mass function is fitted well with a power-law function with an index of 2.3. Although two sequences of self-gravitating and diffuse clouds are expected to appear in the M_tot_-M_H2_ diagram according to previous works based on a plane-parallel model, the observational data show only a single sequence with large scattering within these two sequences. This implies that most of the clouds are mixtures of these two types of clouds. Moreover, we suggest the following scenario of molecular-gas formation: an HI-dominant cloud evolved with increasing H2 mass along a path of M_H2_{prop.to}M^2^_tot_ by collecting diffuse gas before reaching and moving along the curves of the two sequences.</description><source format="bibcode">2020PASJ...72...43N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/72/43</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/J/AJ/122/3155">J/AJ/122/3155 : Peculiar HI cloud near galactic plane (Higgs+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/626/887">J/ApJ/626/887 : HI clouds in Southern Galactic Plane Survey (Kavars+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/367">J/ApJ/722/367 : HI clouds in Quadrant I of the Milky Way (Ford+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/L4">J/ApJ/770/L4 : HI clouds around the Galactic Center (McClure-Griffiths+, 2013)</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/72/43</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASJ/72/43</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASJ/72/43</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASJ/72/43</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/PASJ/72/43</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASJ/72/43</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/72/43/table1 (Identified HI clouds)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASJ/72/43/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/PASJ/72/43/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASJ/72/43/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>288.6395</ra><dec>9.9369</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/7382-7383 7554 7561 7564 7567 7578-7579 7604-7605 7648 7651 7654 7661 7672-7673 6/29509 29511 29517 29520 29522-29523 29526-29527 29557 30222-30223 30234 30240-30241 30243 30260 30262-30265 30306-30307 30328 30330-30331 30334 30401 30404-30405 30428-30429 30598-30601 30603 30610 30620 30622-30623 30629 30640-30641 30666-30667 30697 30700-30701</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/PASJ/72/43?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/PASJ/72/43/table1</name><description>Identified HI clouds</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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