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Sinks of Light Elements in Stars - Part II

Published online by Cambridge University Press:  25 May 2016

Marc H. Pinsonneault ,
Corinne Charbonnel  and
Constantine P. Deliyannis
Marc H. Pinsonneault
Affiliation:
The Ohio State University, Department of Astronomy, 140 W. 18th Ave. Columbus, Ohio 43210, USA
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

Abstract

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See the abstract given in Part I (Deliyannis, Pinsonneault, Charbonnel, hereafter DPC, in these proceedings). In Part II we discuss the lithium data for metal-poor stars and the constraints it places on stellar depletion. There are a variety of indicators that place interesting bounds on the degree of stellar depletion, and in contrast to the other two sections the data for Population II stars provides weaker evidence for stellar lithium depletion. We review both the theoretical studies and the observational data, and critically evaluate the degree of stellar depletion consistent with the data.

Information

Type
2. Production and Destruction of the Elements
Information
Symposium - International Astronomical Union , Volume 198: The Light Elements and their Evolution , 2000 , pp. 74 - 86
Copyright
Copyright © Astronomical Society of the Pacific 2000 

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