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Evolution of Stars with M 8 M ⊙

Published online by Cambridge University Press:  14 August 2015

B. Paczyński
B. Paczyński*
Affiliation:
Institute of Astronomy, Polish Academy of Sciences, Warsaw, Poland

Abstract

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The late stages of evolution of stars that develop degenerate carbon-oxygen cores are discussed. Model computations indicate that the initial masses of such stars, M, are below M 1 = 8 M ⊙ ± ± 2 M ⊙. The low mass stars (M < M 0) lose their envelopes and become white dwarfs. The intermediate stars (M 0 < M < M 1) ignite carbon in their highly degenerate cores of 1.4 M ⊙. Present observational and/or theoretical estimates of M 0 are very uncertain. Problems associated with mass loss and with carbon ignition and burning are discussed.

Information

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 66: Late Stages of Stellar Evolution , 1974 , pp. 62 - 69
Copyright
Copyright © Reidel 1974 

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