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<ri:Resource created="2014-01-15T09:48:06Z" 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>Far-UV spectra of Galactic corona sight lines</title><shortName>J/ApJ/749/157</shortName><identifier>ivo://CDS.VizieR/J/ApJ/749/157</identifier><altIdentifier>doi:10.26093/cds/vizier.17490157</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wakker B.P.</name></creator><creator><name>Savage B.D.</name></creator><creator><name>Fox A.J.</name></creator><creator><name>Benjamin R.A.</name></creator><creator><name>Shapiro P.R.</name></creator><date role="Updated">2018-01-04T08:22:40Z</date><date role="Created">2014-01-15T09:48:06Z</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>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>interstellar-medium</subject><subject>milky-way-galaxy</subject><description>We present a study of the properties of the transition temperature (T~10^5^K) gas in the Milky Way corona, based on the measurements of OVI, NV, CIV, SiIV, and FeIII absorption lines seen in the far-ultraviolet spectra of 58 sight lines to extragalactic targets, obtained with the Far-Ultraviolet Spectroscopic Explorer and the Space Telescope Imaging Spectrograph. In many sight lines the Galactic absorption profiles show multiple components, which are analyzed separately. We find that the highly ionized atoms are distributed irregularly in a layer with a scale height of about 3 kpc, which rotates along with the gas in the disk, without an obvious gradient in the rotation velocity away from the Galactic plane. Within this layer the gas has randomly oriented velocities with a dispersion of 40-60km/s. On average the integrated column densities are logN(OVI)=14.3, logN(NV)=13.5, logN(CIV)=14.2, logN(SiIV)=13.6, and logN(FeIII)=14.2, with a dispersion of just 0.2 dex in each case. In sight lines around the Galactic center and Galactic north pole, all column densities are enhanced by a factor ~2, while at intermediate latitudes in the southern sky there is a deficit in N(O VI) of about a factor of two, but no deficit for the other ions.</description><source format="bibcode">2012ApJ...749..157W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/749/157</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/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/129">VI/129 : The FUSE Observation Log (FUSE, 1999-2007)</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/J/ApJS/182/378">J/ApJS/182/378 : HI and OVI absorbers in nearby Universe (Wakker+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/702/1472">J/ApJ/702/1472 : Column densities for HI, AlIII, SiIV, CIV, OVI (Savage+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/176/59">J/ApJS/176/59 : FUSE survey of OVI in the disk of the Milky Way (Bowen+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/168/213">J/ApJS/168/213 : Ionization states and cooling efficiencies (Gnat+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/647/312">J/ApJ/647/312 : FUSE survey of OVI in the Milky Way (Otte+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/163/282">J/ApJS/163/282 : Molecular hydrogen column densities (Wakker+, 2006)</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/ApJS/146/1">J/ApJS/146/1 : O VI absorption in FUSE survey (Wakker+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/136/631">J/ApJS/136/631 : IUE absorption toward 164 early-type stars (Savage+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/136/463">J/ApJS/136/463 : Distances and metallicities of HVCs and IVCs (Wakker, 2001)</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/749/157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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