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Lithium Depletion in a [Fe/H]= —3.4 star?

Published online by Cambridge University Press:  25 May 2016

M. Spite ,
F. Spite ,
R. Cayrel ,
V. Hill ,
E. Depagne ,
B. Nordström  and
T.C. Beers
M. Spite
Affiliation:
Observatoire de Paris-Meudon, CNRS UMR 8633, F-92195 Meudon Cedex, France
F. Spite
Affiliation:
Observatoire de Paris-Meudon, CNRS UMR 8633, F-92195 Meudon Cedex, France
R. Cayrel
Affiliation:
Observatoire de Paris-Meudon, CNRS UMR 8633, F-92195 Meudon Cedex, France
V. Hill
Affiliation:
ESO, Garching bei Miinchen, D-85748, Germany
E. Depagne
Affiliation:
Observatoire de Paris-Meudon, F-92195 Meudon Cedex, France
B. Nordström
Affiliation:
Niels Bohr Institute, DK-2100 Copenhagen, Denmark
T.C. Beers
Affiliation:
Michigan State University, Dept of Phys. and Astronomy, USA

Abstract

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We present a determination of the lithium abundance from high quality spectra in an extremely metal poor star where the lithium line had not been detected.

Type
4. Lithium Abundances
Information
Symposium - International Astronomical Union , Volume 198: The Light Elements and their Evolution , 2000 , pp. 356 - 357
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

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