Expanding envelopes of binary stars. II - Motion in extremely hot envelopes

Details Expanding envelopes of binary stars. II - Motion in extremely hot envelopes Expanding envelopes of binary stars. II - Motion in extremely hot envelopes

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.110..257n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 110, no. 2, March 1985, p. 257-276.

Astronomy and Astrophysics

Astrophysics

4

Binary Stars, High Temperature Plasmas, Stellar Envelopes, Stellar Mass Ejection, Stellar Models, Stellar Motions, Euler Equations Of Motion, Hamilton-Jacobi Equation, Mass Distribution, Particle Motion, Stellar Winds, Velocity Distribution

Scientific paper

In this paper, which is a continuation of Neutsch and Schmidt (1985), the authors investigate the structure of binary envelopes under the hypothesis that at least one of the companions produces a very intense radiation field. The limiting case in which the forces due to the system's rotation (i. e., Coriolis and centrifugal forces) as well as gas pressure can be neglected is solved analytically using a classical result of Euler. Beyond this the velocity and density distributions in the envelope are determined.

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