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Heating of the intracluster medium by quasar outflows

dc.contributor.authorRoychowdhury, Suparna
dc.contributor.authorNath, Biman B
dc.date.accessioned2005-12-26T05:05:17Z
dc.date.available2005-12-26T05:05:17Z
dc.date.issued2002
dc.description.abstractWe study the possibility of quasar outflows in clusters and groups of galaxies heating the intracluster gas in order to explain the recent observation of excess entropy in this gas. We show that radio galaxies alone cannot provide the energy required to explain the observations but the inclusion of Broad Absorption Line (BAL) outflows can do so, and that in this scenario most of the heating takes place at z ~ 1-4, the ``preheating'' epoch being at a lower redshift for lower mass clusters.en
dc.format.extent56004 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationJournal of Astrophysics and Astronomy, 2002, Vol. 23, p101-105.en
dc.identifier.issn0250-6335
dc.identifier.urihttp://hdl.handle.net/2289/817
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.subjectCosmology-theoryen
dc.subjectGalaxiesen
dc.subjectInter galactic mediumen
dc.subjectX-raysen
dc.subjectGalaxiesen
dc.subjectClustersen
dc.titleHeating of the intracluster medium by quasar outflowsen
dc.typeArticleen

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