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Circulation and Mixing

Published online by Cambridge University Press:  14 August 2015

R. Kippenhahn
R. Kippenhahn*
Affiliation:
Universitäts-Sternwarte, Göttingen, F.R.G.

Extract

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In the preceding lecture Dr Arnett has shown us how exciting the inner life of a star can be when during late stages of evolution higher nuclear reactions take place. But in order to enjoy the variety of different nuclear species formed there stellar material from the deep interior has to be brought up to the surface, where the observers can see it.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 66: Late Stages of Stellar Evolution , 1974 , pp. 20 - 40
Copyright
Copyright © Reidel 1974 

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