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<ri:Resource created="2015-09-17T10:52:07Z" 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>HST/COS observations of QSOs within 600kpc of M31</title><shortName>J/ApJ/804/79</shortName><identifier>ivo://CDS.VizieR/J/ApJ/804/79</identifier><altIdentifier>doi:10.26093/cds/vizier.18040079</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lehner N.</name></creator><creator><name>Howk J.C.</name></creator><creator><name>Wakker B.P.</name></creator><date role="Updated">2017-12-07T07:27:46Z</date><date role="Created">2015-09-17T10:52:07Z</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>galaxies</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>quasars</subject><description>We demonstrate the presence of an extended and massive circumgalactic medium (CGM) around Messier 31 using archival HST Cosmic Origins Spectrograph ultraviolet spectroscopy of 18 QSOs projected within two virial radii of M31 (R_vir_=300kpc). We detect absorption from SiIII at -300&lt;~V_LSR_&lt;~-150km/s toward all three sightlines at R&lt;~0.2R_vir_, 3 of 4 sightlines at 0.8&lt;~R/R_vir_&lt;~1.1, and possibly 1 of 11 at 1.1&lt;R/R_vir_&lt;~1.8. We present several arguments that the gas at these velocities observed in these directions originates from the M31 CGM rather than the Local Group or Milky Way CGM or Magellanic Stream. We show that the dwarf galaxies located in the CGM of M31 have very similar velocities over similar projected distances from M31. We find a non-trivial relationship only at these velocities between the column densities (N) of all the ions and R, whereby N decreases with increasing R. At R&lt;0.8R_vir_, the covering fraction is close to unity for Si III and C IV (f_c_~60%-97% at the 90% confidence level), but drops to f_c_&lt;~10%-20% at R&gt;~R_vir_. We show that the M31 CGM gas is bound, multiphase, predominantly ionized, and is more highly ionized gas at larger R. We estimate using Si II, Si III, and Si IV, a CGM metal mass of &gt;~2x10^6^M_{sun}_ and gas mass of &gt;~3x10^9^(Z_{sun}_/Z)M_{sun}_ within 0.2R_vir_, and possibly a factor of ~10 larger within R_vir_, implying substantial metal and gas masses in the CGM of M31.</description><source format="bibcode">2015ApJ...804...79L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/804/79</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/A+A/567/A71">J/A+A/567/A71 : M31 Herschel images (Viaene+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/445/2061">J/MNRAS/445/2061 : Absorption in multiphase CGM (Liang+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/138">J/ApJ/770/138 : Metallicities of Lyman limit systems and DLA (Lehner+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/133">J/ApJ/758/133 : Metallicity profile of M31 HII region &amp; PN (Sanders+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/4">J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)</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/ApJ/745/156">J/ApJ/745/156 : M31 Cepheids with HST/WFC3 (Riess+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/91">J/ApJ/740/91 : Ly{alpha} &amp; OVI in galaxies around QSOs (Prochaska+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/415/1105">J/MNRAS/415/1105 : Intermediate high-velocity clouds distances (Smoker+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/727/46">J/ApJ/727/46 : Highly ionized plasmas in the Milky Way (Lehner+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/714/1521">J/ApJ/714/1521 : Spectroscopy of galaxies around distant QSOs (Chen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/399/728">J/MNRAS/399/728 : UV-bright sources behind M31 halo (Fittingoff+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/614">J/ApJ/703/614 : UV star-forming regions in M31 (Kang+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/702/940">J/ApJ/702/940 : Radio and UV spectra of HVC toward the MC (Lehner+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/1299">J/ApJ/700/1299 : Gas-phase element depletions in the ISM (Jenkins, 2009)</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/ApJS/168/213">J/ApJS/168/213 : Ionization states and cooling efficiencies (Gnat+, 2007)</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/A+A/417/421">J/A+A/417/421 : WSRT wide-field HI survey. 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