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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4115
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dc.contributor.authorShubhrangshu, Ghosh-
dc.contributor.authorMukhopadhyay, Banibrata-
dc.contributor.authorKrishnan, Vinod-
dc.contributor.authorManoranjan, Khan-
dc.date.accessioned2011-08-23T09:17:19Z-
dc.date.available2011-08-23T09:17:19Z-
dc.date.issued2010-01-
dc.identifier.citationNew Astronomy, 2010, Vol.14, p83en
dc.identifier.issn1384-1076-
dc.identifier.urihttp://hdl.handle.net/2289/4115-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractWe study the energetics of the accretion-induced outflow and then plausible jet around black holes/compact objects using a newly developed disc-outflow coupled model. Inter-connecting dynamics of outflow and accretion essentially upholds the conservation laws. The energetics depend strongly on the viscosity parameter a and the cooling factor f which exhibit several interesting features. The bolometric luminosities of ultra-luminous X-ray binaries (e.g. SS433) and family of highly luminous AGNs and quasars can be reproduced by the model under the super-Eddington accretion flows. Under appropriate conditions, lowluminous AGNs (e.g. Sagittarius A ) also fit reasonably well with the luminosity corresponding to a sub- Eddington accretion flow with f ! 1.en
dc.language.isoenen
dc.publisherElesvier B.V.en
dc.relation.urihttp://adsabs.harvard.edu/abs/2010NewA...15...83Gen
dc.relation.urihttp://arxiv.org/abs//0906.0149en
dc.relation.urihttp://dx.doi.org/10.1016/j.newast.2009.05.012en
dc.rights2010 Elesvier B.V.en
dc.subjectAccretion discen
dc.subjectBlack hole physicsen
dc.subjectX-ray binariesen
dc.subjectGalaxies: jetsen
dc.subjectGalaxies: nucleien
dc.titleDescription of accretion induced outflows from ultra-luminous sources to under luminous AGNsen
dc.typeArticleen
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