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Sinks of Light Elements in Stars - Part III

Published online by Cambridge University Press:  25 May 2016

Corinne Charbonnel ,
Constantine P. Deliyannis  and
Marc H. Pinsonneault
Corinne Charbonnel
Affiliation:
Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées, CNRS-UMR 5572, 14, av. E. Belin, F-31400 Toulouse, France
Constantine P. Deliyannis
Affiliation:
Indiana University, Astronomy Department, 319 Swain Hall West, 727 E. 3rd Street, Bloomington, IN 47405-7105, USA
Marc H. Pinsonneault
Affiliation:
The Ohio State University, Department of Astronomy, 140 W. 18th Ave., Columbus, OH 43210, USA

Abstract

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See the abstract given in Part I (Deliyannis, Pinsonneault, Charbonnel, hereafter DPC, this volume). In Part III, we first discuss the LiBeB observations in subgiant stars and the constraints they bring on the transport processes occuring on the main sequence. Evidence is then reviewed that suggests that in situ mixing occurs in evolved low mass Population I and Population II stars. Theoretical mechanisms that can create such mixing are discussed, as well as their implications for the evolution of the LiBeB and 3He.

Information

Type
2. Production and Destruction of the Elements
Information
Symposium - International Astronomical Union , Volume 198: The Light Elements and their Evolution , 2000 , pp. 87 - 97
Copyright
Copyright © Astronomical Society of the Pacific 2000 

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