Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1899
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dc.contributor.authorNath, Biman B.-
dc.date.accessioned2007-01-12T06:14:28Z-
dc.date.available2007-01-12T06:14:28Z-
dc.date.issued2003-03-
dc.identifier.citationMonthly Notice of the Royal Astronomical Society, 2003, Vol.339, p721-730.en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/1899-
dc.descriptionRestricted Access. An open access version is available at NASA ADS (alternative location).en
dc.description.abstractWe study steady, homogeneous and subsonic cooling flows in poor clusters of galaxies in light of the recent proposal that radiative cooling of the intracluster gas can explain the observations of the `entropy floor' and other related X-ray observations. We study a family of cooling flow solutions parametrized by the mass flux rate, and then determine the resulting entropy and the X-ray luminosity. We find that cooling flows with mass flux rates in excess of 1000 Msolar yr-1 are required to explain the observations of entropy and X-ray luminosity. In view of the observed lack of such large flows in rich clusters, our calculations suggest that heating sources are needed, in addition to the effect of radiative cooling, to explain the observations.en
dc.format.extent8338 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishing for the Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2003MNRAS.339..721Nen
dc.relation.urihttp://dx.doi.org/10.1046/j.1365-8711.2003.06214.xen
dc.rights(2003) Royal Astronomical Societyen
dc.subjectgalaxies: clusters: generalen
dc.subjectintergalactic mediumen
dc.subjectcosmology: theoryen
dc.subjectX-rays: galaxies: clustersen
dc.titleCooling flows and the entropy of the intragroup mediumen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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