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<ri:Resource created="2023-09-05T16:30:13Z" 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>Milky Way SiIV and CIV kinematics from HST/COS</title><shortName>J/ApJ/924/86</shortName><identifier>ivo://CDS.VizieR/J/ApJ/924/86</identifier><altIdentifier>doi:10.26093/cds/vizier.19240086</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Qu Z.</name></creator><creator><name>Lindley R.</name></creator><creator><name>Bregman J.N.</name></creator><date role="Updated">2023-11-09T13:04:29Z</date><date role="Created">2023-09-05T16:30:13Z</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>intergalactic-medium</subject><subject>milky-way-galaxy</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>active-galactic-nuclei</subject><description>We compose a 265-sight-line Milky Way CIV line-shape sample using the Hubble Space Telescope/Cosmic Origins Spectrograph archive, which is complementary to the existing SiIV samples. CIV has a higher ionization potential (47-64eV) than SiIV (33-45eV), so it also traces warm gas, which is roughly cospatial with SiIV. The spatial density distribution and kinematics of CIV are identical to those SiIV within ~2{sigma}. CIV is more sensitive to the warm gas density distribution at large radii with a higher element abundance. Applying the kinematical model to the CIV sample, we find two possible solutions of the density distribution, which are distinguished by the relative extension along the disk midplane and the normal-line direction. Both solutions can reproduce the existing sample and suggest a warm gas disk mass of logM(M_{sun}_)~8 and an upper limit of logM(M_{sun}_)&lt;9.3 within 250kpc, which is consistent with SiIV. There is a decrease in the CIV/SiIV column density ratio from the Galactic center to the outskirts by 0.2-0.3dex, which may suggest a phase transition or different ionization mechanisms for CIV and SiIV. Also, we find that the difference between CIV and SiIV is an excellent tracer of small-scale features, and we find a typical size of 5{deg}-10{deg} for possible turbulence within individual clouds (~1kpc).</description><source format="bibcode">2022ApJ...924...86Q</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/924/86</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/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/168/213">J/ApJS/168/213 : Ionization states and cooling efficiencies (Gnat+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/176/59">J/ApJS/176/59 : FUSE survey of OVI in the disk of the MW (Bowen+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/702/1472">J/ApJ/702/1472 : HI, AlIII, SiIV, CIV, OVI column densities (Savage+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/749/157">J/ApJ/749/157 : FUV spectra of Galactic corona sight lines (Wakker+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/21">J/ApJS/217/21 : XMM-Newton survey of local OVII absorbers (Fang+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/814/40">J/ApJ/814/40 : Nearby galaxy filaments with UV obs. (Wakker+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/228/11">J/ApJS/228/11 : Time-dependent cooling in photoionized plasma (Gnat, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/478/4513">J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/871/35">J/ApJ/871/35 : HST/COS spectra of QSOs with SiIV data (Zheng+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/NatAs/4.1072">J/other/NatAs/4.1072 : HaloSat survey of southern Galactic halo (Kaaret+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/900/9">J/ApJ/900/9 : AMIGA: Circumgalactic Medium of Andromeda (Lehner+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/894/142">J/ApJ/894/142 : Column densities from COS SiIV AGN sight lines (Qu+, 2020)</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/924/86</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/924/86</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/924/86</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/924/86</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/924/86</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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