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<ri:Resource created="2023-12-04T11:38:56Z" status="active" updated="2026-07-02T11:58:25Z" 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>GASKAP pilot survey science. II. 21cm abs.</title><shortName>J/ApJ/926/186</shortName><identifier>ivo://CDS.VizieR/J/ApJ/926/186</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-wy-5t</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dickey J.M.</name></creator><creator><name>Dempsey J.M.</name></creator><creator><name>Pingel N.M.</name></creator><creator><name>McClure-Griffiths N.M.,Jameson K.</name></creator><creator><name>Dawson J.R.</name></creator><creator><name>Denes H.</name></creator><creator><name>Clark S.E.</name></creator><creator><name>Joncas G.</name></creator><creator><name>Leahy D.,Lee M.-Y.</name></creator><creator><name>Miville-Deschenes M.-A.</name></creator><creator><name>Stanimirovic S.</name></creator><creator><name>Tremblay C.D.,van Loon J.T.</name></creator><date role="Updated">2026-07-02T11:58:25Z</date><date role="Created">2023-12-04T11:38:56Z</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>interstellar-medium</subject><subject>radio-astronomy</subject><subject>milky-way-galaxy</subject><description>Using the Australian Square Kilometre Array Pathfinder to measure 21cm absorption spectra toward continuum background sources, we study the cool phase of the neutral atomic gas in the far outer disk, and in the inner Galaxy near the end of the Galactic bar at longitude 340{deg}. In the inner Galaxy, the cool atomic gas has a smaller scale height than in the solar neighborhood, similar to the molecular gas and the super-thin stellar population in the bar. In the outer Galaxy, the cool atomic gas is mixed with the warm, neutral medium, with the cool fraction staying roughly constant with the Galactic radius. The ratio of the emission brightness temperature to the absorption, i.e., 1-e^-{tau}^, is roughly constant for velocities corresponding to Galactic radius greater than about twice the solar circle radius. The ratio has a value of about 300K, but this does not correspond to a physical temperature in the gas. If the gas causing the absorption has kinetic temperature of about 100K, as in the solar neighborhood, then the value 300 K indicates that the fraction of the gas mass in this phase is one-third of the total HI mass.</description><source format="bibcode">2022ApJ...926..186D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/926/186</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/B/psr">B/psr : ATNF Pulsar Catalogue (Manchester+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/76">VIII/76 : Leiden/Argentine/Bonn (LAB) Survey of Galactic HI (Kalberla+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/284">VII/284 : A Catalogue of Galactic Supernova Remnants (Green, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/76/317">J/A+AS/76/317 : Possible new PNe in IRAS PSC (Preite-Martinez, 1988)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/275/67">J/A+A/275/67 : Velocity Field of the outer Galaxy (Brand+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/649/759">J/ApJ/649/759 : Bubbles in the galactic disk (Churchwell+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/783/130">J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/793/132">J/ApJ/793/132 : Perseus cloud sources Gaussian param. 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