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Evolutionary effects of mass loss in low-mass stars

Published online by Cambridge University Press:  12 April 2016

Alvio Renzini
Alvio Renzini*
Affiliation:
Osservatorio Astronomico, CP 596, 40100 Bologna, Italy

Abstract

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The effects of mass loss on the evolution of low-mass stars (actual mass smaller than 1.4 Mʘ) are reviewed. The case of globular cluster stars is discussed in some detail, and it is shown that evolutionary theory sets quite precise limits to the mass-loss rate in population II red giants. The effects of mass loss on the final evolutionary stages of stars producing white dwarfs is also discussed. In particular, the interaction of the wind from the hot central star with the surrounding planetary nebula is considered. Finally, the problem of the origin of hydrogen-deficient stars is briefly discussed.

Type
Session VI - Mass Loss and Stellar Evolution: Low Mass Stars
Information
International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 319 - 338
Copyright
Copyright © Reidel 1981

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