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Stellar Wind Equations in a New Steady State

Published online by Cambridge University Press:  12 April 2016

Mariko Kato
Mariko Kato*
Affiliation:
Department of Astronomy, Keio UniversityHiyoshi, Kouhoku-ku Yokohama 223Japan

Abstract

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A set of equations of stellar wind in a new steady state in spherically symmetry is presented. This equations are available also for the deep interior of stars, whereas the usual equations can be applied only to the surface region. The new equations have a variable mass flux which becomes zero at the inner boundary of the mass flow. The velocity also reduces zerj), whereas it diverges at r=0 in the usual continuity equation 4∏r2ρ v=constant. In the surface region, the present equations approach the usual equations.

Type
Part II. Mass-Losing Stars in Different Stages of Evolution
Information
International Astronomical Union Colloquium , Volume 108: Atmospherics Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion , 1988 , pp. 156 - 157
Copyright
Copyright © Springer-Verlag 1988

References

Kato, M., 1983a, Publ. Astron. Soc. Japan, 35, 33 Google Scholar
Kato, M., 1983b, Publ. Astron. Soc. Japan, 35, 507 Google Scholar
Kato, M., 1986, Publ. Astron. Soc. Japan, 38, 29.Google Scholar