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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1542
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dc.contributor.authorEnsslin, T.A.-
dc.contributor.authorWang, Yiping-
dc.contributor.authorNath, Biman B.-
dc.contributor.authorBiermann, P.L.-
dc.date.accessioned2006-11-24T11:21:15Z-
dc.date.available2006-11-24T11:21:15Z-
dc.date.issued1998-05-
dc.identifier.citationAstronomy and Astrophysics, 1998, Vol.333, pL47-L50en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2289/1542-
dc.description.abstractWe estimate the energy release of black hole formation to the intra-cluster medium of the Coma cluster and find that this is comparable to the present day energy content. Therefore an energetic and maybe hydrostatic influence is possible. Our calculations rely on the assumption of an universal black hole to galaxy mass ratio (more exactly: spheroidal mass component of the stellar population), for which there is growing evidence. On a cosmological scale, there is also an energy release of black hole formation comparable to what is expected to be present within the thermal gas, caused by the process of structure formation. This indicates an important dynamical influence, neglected by present day structure formation simulations. This estimate of cosmological black hole energy release is independent of the black hole to galaxy mass ratio, but consistent with its value.en
dc.format.extent105296 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringer-Verlagen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998A%26A...333L..47E&link_type=ARTICLE&db_key=ASTen
dc.relation.urihttp://arxiv.org/abs/astro-ph/9803105en
dc.rights(1998) by European Southern Observatoryen
dc.subjectBLACK HOLE PHYSICSen
dc.subjectINTERGALACTIC MEDIUMen
dc.subjectGALAXIES: JETSen
dc.subjectGALAXIES: CLUSTERS: INDIVIDUAL: COMAen
dc.subjectCOSMOLOGY: LARGE-SCALE STRUCTURE OF THE UNIVERSEen
dc.titleBlack hole energy release to the Gaseous Universeen
dc.typeArticleen
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