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

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

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..268..489m&link_type=abstract

Light Elements in the Universe, Proceedings of the International Astronomical Union, IAU Symposium, Volume 268, p. 489-492

Astronomy and Astrophysics

Astronomy

Nucleosynthesis, Abundances

Scientific paper

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.

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