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Bondi flow revisited

Authors
  • Datta, Satadal
Type
Preprint
Publication Date
Jan 06, 2016
Submission Date
Jan 06, 2016
Identifiers
DOI: 10.1007/s10509-016-2849-2
Source
arXiv
License
Yellow
External links

Abstract

Newtonian spherically symmetric transonic accretion has been studied by including the mass of the accreting matter, while considering the growth of the accretor itself to be negligibly small. A novel iterative method has been introduced to accomplish that task. It has been demonstrated that the inclusion of the mass of the fluid changes the critical properties of the flow as well as the topological phase portraits of the stationary integral solution.

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