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Properties of optically thick winds driven by radiation pressure

Published online by Cambridge University Press:  12 April 2016

M. Friedjung
M. Friedjung*
Affiliation:
Institut d'Astrophysique, CNRS, Paris, France

Abstract

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Conditions are derived for supercritical winds, accelerated by the radiation pressure of an object above the Eddington limit. A relation between the different energy fluxes is found. The conditions seem to be satisfied by novae, and perhaps by η Car. They are not satisfied however by the symbiotic star Z And.

Type
Session VIII - Effects of Mass Loss on the Evolution of Binary Stars
Information
International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 495 - 497
Copyright
Copyright © Reidel 1981

References

Andriesse, CD., Dorm, B.D., Viotti, R.: 1978, Mon. Not. R.A.S. 185, 771.CrossRefGoogle Scholar
Bath, G.T.: 1977, Mon. Not. R.A.S. 178, 203.CrossRefGoogle Scholar
Bath, G.T.: 1978, Mon. Not. R.A.S. 182, 35.CrossRefGoogle Scholar
Bath, G.T.: 1979, Nature 282, 274.CrossRefGoogle Scholar
Bath, G.T., Shaviv, G.: 1976, Mon. Not. R.A.S. 175, 305.CrossRefGoogle Scholar
Friedjung, M.: 1966, Mon. Not. R.A.S. 132, 317.CrossRefGoogle Scholar
Friedjung, M.: 1980, being submitted.Google Scholar
Ruggles, C.L.N., Bath, G.T.: 1979, Astr. Astrophys. 80, 97.Google Scholar