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DICUSSION C. The stellar yields in He-3, He-4 and Li-7: main sources, observational constraints, and problems

Published online by Cambridge University Press:  23 April 2010

André Maeder
André Maeder*
Affiliation:
Geneva Observatory, University of Geneva, CH-1290 Versoix, Switzerland email: [email protected]
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I am pleased to recall that the first determination of the Li–abundance in the Sun was made at the Geneva Observatory in 1975 by Edith Müller, Eric Peytremann and Ramiro de la Reza on the basis of spectra taken at Kitt Peak. The first Be determination was also made in Geneva the same year by Y. Chmielewski, J. Brault (Kitt Peak National Observatory) and E. Müller. These two outstanding works opened the door for all further investigations on these light elements.

Keywords

Nucleosynthesisabundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S268: Light Elements in the Universe , November 2009 , pp. 489 - 492
Copyright
Copyright © International Astronomical Union 2010