Similarity Solution for Unsteady Accretion Flow, II

Details Similarity Solution for Unsteady Accretion Flow, II Similarity Solution for Unsteady Accretion Flow, II

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..31..251s&link_type=abstract

Astrophysics and Space Science, Volume 31, Issue 1, pp.251-259

Astronomy and Astrophysics

Astrophysics

12

Scientific paper

Similarity solution for unsteady accretion flow is obtained. The density distribution of the initial state of the gas surrounding the star is given as ϱ0 ∝r -ω. The flow patterns are compared with the results of the numerical computation by Zel'dovichet al. (1972), and it is shown that the similarity solution reproduces the results of the numerical computations well. An unsteady accretion model for the nova-like X-ray source is discussed briefly.

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