Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5573
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dc.contributor.authorSharma, Mahavir-
dc.contributor.authorNath, Biman B.-
dc.contributor.authorChand, Hum-
dc.date.accessioned2013-05-06T09:30:52Z-
dc.date.available2013-05-06T09:30:52Z-
dc.date.issued2013-04-01-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society : Letters, 2013, 431, L93-L97en
dc.identifier.issn1745-3933 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/5573-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractWe report a correlation between velocity offset (β = v/c) of strong Mg ii absorption systems and the bolometric luminosity (Lbol) of quasars in SDSS-DR7. We find that β shows a power-law increase with Lbol, with a slope ∼1/4. We find that such a relation of β with Lbol is expected for outflows driven by scattering of black hole radiation by dust grains, and which are launched from the innermost dust survival radius. Our results indicate that a significant fraction of the strong Mg ii absorbers, in the range of β = 0–0.4, may be associated with the quasars themselves.en
dc.language.isoenen
dc.publisherOxford University Press for the RASen
dc.relation.urihttp://adsabs.harvard.edu/abs/2013MNRAS.431L..93Sen
dc.relation.urihttp://arxiv.org/abs/1212.3755en
dc.relation.urihttp://dx.doi.org/10.1093/mnrasl/slt015en
dc.rights2013 The authors & the Royal Astronomical Society.en
dc.subjectISMen
dc.subjectjets and outflows galaxiesen
dc.subjectactive quasarsen
dc.subjectabsorption linesen
dc.subjectquasars - Generalen
dc.titleSignature of outflows in strong Mg  II absorbers in quasar sightlinesen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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