Supersonic flow past weak radiation sources

Details Supersonic flow past weak radiation sources Supersonic flow past weak radiation sources

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izssr......133k&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Mekhanika Zhidkosti i Gaza (ISSN 0568-5281), July-Aug. 1984, p. 133-136. In Russian.

Physics

Gas Dynamics, Radiation Sources, Stellar Winds, Supersonic Flow, X Ray Sources, Flow Distribution, Flow Equations

Scientific paper

The supersonic flow of a stellar wind past an X-ray source is considered. A qualitative analogy between the supersonic flow past nonporous bodies and radiation sources leads to the hypothesis that a shock wave that does not intersect the symmetry axis can arise in the case of a low energy emission power. Conditions under which this can occur are described, and a quantitative analogy between the supersonic flow past thin bodies and radiation sources is established. Also determined is the flow region where this analogy does not hold.

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