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What Theorists Think They Know about AGB Stars

Published online by Cambridge University Press:  25 May 2016

John C. Lattanzio
John C. Lattanzio*
Affiliation:
Department of Mathematics, Monash University, Clayton, VIC 3168, Australia

Abstract

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In this paper I discuss our basic picture of the structure of AGB stars, and how their earlier evolution led them to this situation.

Information

Type
Introduction
Information
Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 7 - 9
Copyright
Copyright © Kluwer 2000 

References

Boothroyd, A. I. & Sackmann, I.-J. 1992, ApJ, 393, L21 Google Scholar
Frost, C. A. & Lattanzio, J. C. 1996, in Stellar Evolution: What Should Be Done?, Proceedings of the 32nd Liège Colloquium, ed. Noels, A. et al., p. 307 Google Scholar
Lattanzio, J.C., Frost, C. A., Cannon, R. C. & Wood, P. R. 1996, Mem. Astron. Soc. Italia, 67, 729 Google Scholar
Mowlavi, N., Jorissen, A. & Arnould, M. 1996, A&A, 311, 803 Google Scholar
Straniero, O., Gallino, R., Busso, M., Chieffi, A., Raiteri, C. M., Limongi, M. & Salaris, M. 1995, ApJ, 440, L85 CrossRefGoogle Scholar
Wood, P. R., Bessell, M. S. & Fox, M. W. 1983, ApJ, 272, 99 Google Scholar
Zinner, E. K. 1995, in Nuclei in the Cosmos III, ed. Busso, M., Gallino, R. and Raiteri, C. M. (AIP Press: New York), p. 567 Google Scholar