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Analytic solutions to the accretion of a rotating finite cloud towards a central object I. Newtonian approach.

By S. Mendoza, E. Tejeda and E. Nagel

Abstract

The first model of a spherical symmetric accretion flow towards a central object was made by Bondi (1952). With time, it has become the key to understand different accretion processes in the universe (see e.g. Frank et al. (2002))

Year: 2008
OAI identifier: oai:CiteSeerX.psu:10.1.1.313.9206
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