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<ri:Resource created="2013-03-12T17:06:03Z" 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>Ly{alpha} and OVI in galaxies around quasars</title><shortName>J/ApJ/740/91</shortName><identifier>ivo://CDS.VizieR/J/ApJ/740/91</identifier><altIdentifier>doi:10.26093/cds/vizier.17400091</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Prochaska J.X.</name></creator><creator><name>Weiner B.</name></creator><creator><name>Chen H.-W.</name></creator><creator><name>Mulchaey J.</name></creator><creator><name>Cooksey K.</name></creator><date role="Updated">2017-11-28T13:21:58Z</date><date role="Created">2013-03-12T17:06:03Z</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><subject>redshifted</subject><subject>line-intensities</subject><description>We analyze the association of galaxies with Ly{alpha} and OVI absorption, the most commonly detected transitions of the low-z intergalactic medium (IGM), in the fields of 14 quasars with z_em_=0.06-0.57. Confirming previous studies, we observe a high covering fraction for Ly{alpha} absorption to impact parameter {rho}=300h^-1^_72_kpc: 33/37 of our L&gt;0.01L* galaxies show Ly{alpha} equivalent width W^Ly{alpha}^&gt;=50 m{AA}. Galaxies of all luminosity L&gt;0.01L* and spectral type are surrounded by a diffuse and ionized circumgalactic medium (CGM), whose baryonic mass is estimated at ~10^10.5^+/-0.3M_{sun}_ for a constant N_H_=10^19^cm^-2^. The virialized halos and extended CGM of present-day galaxies are responsible for most strong Ly{alpha} absorbers (W^Ly{alpha}^&gt;300m{AA}) but cannot reproduce the majority of observed lines in the Ly{alpha} forest. We conclude that the majority of Ly{alpha} absorption with W^Ly{alpha}^=30-300m{AA} occurs in the cosmic web predicted by cosmological simulations and estimate a characteristic width for these filaments of ~400h^-1^_72_kpc. Regarding OVI, we observe a near unity covering fraction to {rho}=200h^-1^_72_kpc for L&gt;0.1L* galaxies and to {rho}=300h^-1^_72_kpc for sub-L* (0.1 L*&lt;L&lt;L*) galaxies. Similar to our Ly{alpha} results, stronger OVI systems (W^1031^&gt;70m{AA}) arise in the virialized halos of L&gt;0.1L* galaxies. Unlike Ly{alpha}, the weaker OVI systems (W^1031^~30m{AA}) arise in the extended CGM of sub-L* galaxies. The majority of OVI gas observed in the low-z IGM is associated with a diffuse medium surrounding individual galaxies with L~0.3L* and rarely originates in the so-called warm-hot IGM (predicted by cosmological simulations.</description><source format="bibcode">2011ApJ...740...91P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/740/91</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/ApJS/193/28">J/ApJS/193/28 : Galaxy survey around 20 UV-bright quasars (Prochaska+, 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/ApJ/701/1219">J/ApJ/701/1219 : Galaxy survey in 3 QSO fields (Chen+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/177/39">J/ApJS/177/39 : Survey of low-redshift OVI absorbers (Tripp+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/679/194">J/ApJ/679/194 : Low-z intergalactic medium. III. (Danforth+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/676/262">J/ApJ/676/262 : PKS1302-102 intergalactic absorption system (Cooksey+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/643/680">J/ApJ/643/680 : Imaging &amp; spectroscopy around PKS 0405-123 (Prochaska+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/617/718">J/ApJ/617/718 : Atomic data and EW for PKS 0405-123 (Prochaska+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/559/654">J/ApJ/559/654 : Ly{alpha} absorption systems. V. (Chen+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/498/77">J/ApJ/498/77 : Ly{alpha} absorption systems. III. 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