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Evolution of Unstable Red Giant Envelopes

Published online by Cambridge University Press:  18 September 2017

Y. Tuchman
Y. Tuchman*
Affiliation:
The Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem, Israel

Extract

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Two main observable phenomena are directly connected with the dynamical behaviour of Red Giant (R.G.) envelopes: The variability of Mira stars and Planetary Nebulae (P.N.) ejection.

Type
Section IV: Origin of Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 103: Planetary Nebulae , 1983 , pp. 281 - 289
Copyright
Copyright © Reidel 1983 

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