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<ri:Resource created="2011-01-25T15:38:08Z" 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>GASS HI survey of the lower halo</title><shortName>J/ApJ/688/290</shortName><identifier>ivo://CDS.VizieR/J/ApJ/688/290</identifier><altIdentifier>doi:10.26093/cds/vizier.16880290</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ford H.A.</name></creator><creator><name>McClure-Griffiths N.M.</name></creator><creator><name>Lockman F.J.</name></creator><creator><name>Bailin J.,Calabretta M.R.</name></creator><creator><name>Kalberla P.M.W.</name></creator><creator><name>Murphy T.</name></creator><creator><name>Pisano D.J.</name></creator><date role="Updated">2012-11-13T06:15:05Z</date><date role="Created">2011-01-25T15:38:08Z</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>molecular-clouds</subject><subject>h-i-line-emission</subject><subject>radio-astronomy</subject><subject>surveys</subject><subject>interstellar-medium</subject><description>We have detected over 400 HI clouds in the lower halo of the Galaxy within the pilot region of the Galactic All-Sky Survey (GASS), a region of the fourth quadrant that spans 18{deg} in longitude, 40{deg} in latitude, and is centered on the Galactic equator. These clouds have a median peak brightness temperature of 0.6K, a median velocity width of 12.8km/s, and angular sizes &lt;~1{deg}. The motion of these clouds is dominated by Galactic rotation with a random cloud-to-cloud velocity dispersion of 18km/s. A sample of clouds likely to be near tangent points was analyzed in detail. These clouds have radii on the order of 30pc and a median HI mass of 630M_{sun}_. The population has a vertical scale height of 400pc and is concentrated in Galactocentric radius, peaking at R=3.8kpc. This confined structure suggests that the clouds are linked to spiral features, while morphological evidence that many clouds are aligned with loops and filaments is suggestive of a relationship with star formation. The clouds might result from supernovae and stellar winds in the form of fragmenting shells and gas that has been pushed into the halo rather than from a galactic fountain.</description><source format="bibcode">2008ApJ...688..290F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/688/290</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/75">VIII/75 : HI survey of the sky DE&lt;+25deg (Bajaja+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/73">VIII/73 : HI Parkes All Sky Survey Catalogue (HIPASS) (Meyer+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/54">VIII/54 : Atlas of Galactic Neutral Hydrogen (Hartmann+, 1997)</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/ApJS/146/125">J/ApJS/146/125 : O VI in the galactic halo (Savage+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/873">J/AJ/123/873 : HIPASS high-velocity clouds (Putman+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/140/331">J/ApJS/140/331 : High-velocity HI observations at 21cm (Lockman+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/142/25">J/A+AS/142/25 : High velocity HI Southern Survey (Morras+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/201/495">J/MNRAS/201/495 : HI Survey of Southern Galactic Plane (Strong+ 1982)</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/ApJ/688/290</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/688/290</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/688/290</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/688/290</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/688/290</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/688/290</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/ApJ/688/290/table1 (HI clouds - 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