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Stellar Evolution in the Upper HRD: Theory

Published online by Cambridge University Press:  03 August 2017

Norbert Langer
Norbert Langer*
Affiliation:
Universitäts-Sternwarte Göttingen Geismarlandstrasse 11, D-3400 Göttingen, F.R.G.

Abstract

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Theoretical aspects of the modeling of observable evolutionary phases of massive single stars are reviewed. The SN 1987A progenitor evolution is considered in detail as an example for a star below the WR limit. Formation, structure, evolution, and mass loss of WR stars are discussed, and the impact of supernova research on stellar evolution theory is stressed.

Type
Session VII. Evolution
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 431 - 444
Copyright
Copyright © Kluwer 1991 

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