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

Maeder, André

In: Proceedings of the International Astronomical Union, 2009, vol. 5, no. S268, p. 489-492

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    Titel
    • DICUSSION C. The stellar yields in He-3, He-4 and Li-7: main sources, observational constraints, and problems
    Autor
    • Maeder, André. Geneva Observatory, University of Geneva, CH-1290 Versoix, Switzerland email: andre.maeder@unige.ch
    Dokumententyp
    • Postprint
    Sprache
    • Englisch
    Veröffentlicht in
    • Proceedings of the International Astronomical Union, 2009, vol. 5, no. S268, p. 489-492. Cambridge University Press
    Andere elektronische Ausgabe
    OAI-PMH-ID
    • oai:doc.rero.ch:301484
    Summary
    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