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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4115

Title: Description of accretion induced outflows from ultra-luminous sources to under luminous AGNs
Authors: Shubhrangshu, Ghosh
Mukhopadhyay, Banibrata
Krishnan, Vinod
Manoranjan, Khan
Keywords: Accretion: accretion disc
Black hole physics
X-rays: binaries
Galaxies: jets
Galaxies: nuclei
Issue Date: Jan-2010
Publisher: Elesvier B.V.
Citation: New Astronomy, 2010, Vol.14, p83
Abstract: We 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.
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI: http://hdl.handle.net/2289/4115
ISSN: 1384-1076
Alternative Location: http://adsabs.harvard.edu/abs/2010NewA...15...83G
http://arxiv.org/abs//0906.0149
http://dx.doi.org/10.1016/j.newast.2009.05.012
Copyright: 2010 Elesvier B.V.
Appears in Collections:Research Papers (A&A)

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