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High-resolution spectroscopic observations of two chemically peculiar metal-poor stars: HD 10613 & BD+04°2466

Published online by Cambridge University Press:  09 March 2010

C. B. Pereira  and
N. A. Drake
C. B. Pereira
Affiliation:
Observatório Nacional Rua José Cristino, 77. CEP 20921-400. São Cristóvão. Rio de Janeiro-RJ. Brazil email: claudio@on.br
N. A. Drake
Affiliation:
Sobolev Astronomical Institute, St. Petersburg State University, Universitetski pr. 28, St. Petersburg 198504, Russia email: drake@on.br
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Abstract

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We determined the atmospheric parameters and abundance pattern of two chemically peculiar metal-poor stars: HD 10613 and BD+04°2466 and discuss the nature of these two objects.

Keywords

stars: fundamental parametersstars: Population IIstars: chemically peculiar
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S265: Chemical Abundances in the Universe: Connecting First Stars to Planets , August 2009 , pp. 130 - 131
Copyright
Copyright © International Astronomical Union 2010

References

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