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Evolution from the AGB: Variability

Published online by Cambridge University Press:  07 August 2017

Dimitar D. Sasselov
Dimitar D. Sasselov*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA

Abstract

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Luminous low-mass stars of intermediate T eff – candidates for post-AGB transition objects to PNNi, are all expected to be pulsationally variable. Different modes and their combinations may be involved, leading to a variety of observed behaviour.

Information

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993, pp. 259 - 262
Copyright
Copyright © Kluwer 1993 

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