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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
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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.
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- 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
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