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Mass Loss from Novae and Supernovae

Published online by Cambridge University Press:  30 March 2016

Michael Friedjung
Michael Friedjung*
Affiliation:
Institut d’Astrophysique, 98 bis Bd Arago, F-75014 Paris

Abstract

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The physics of mass loss from these objects is reviewed. Both winds of different types and nearly instantaneous ejection are involved. Supercritical winds driven by the pressure of radiation from an object above the Eddington limit, probably exist for novae after their outbursts. Observations outside the optical region and in particular in the satellite UV have been very important.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 6: Highlights of Astronomy. As presented at the XVIIIth General Assembly of the IAU, 1982 , 1983 , pp. 581 - 592
Copyright
Copyright © Reidel 1983

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