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Determination of [O/Fe] in BD +23 3130 from ESO VLT-UVES observations

Cayrel, R. (author)
Andersen, J. (author)
Barbuy, B. (author)
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Beers, T. C. (author)
Bonifacio, P. (author)
François, P. (author)
Hill, V. (author)
Molaro, P. (author)
Nordström, Birgitta (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Plez, B. (author)
Primas, F. (author)
Spite, F. (author)
Spite, M. (author)
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 (creator_code:org_t)
2001
2001
English.
In: New Astronomy Reviews. - 1872-9630. ; 45:8, s. 533-535
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We report a new determination of [O/Fe, the relative logarithmicabundance of O/Fe with respect to the Sun, for the very metal-poor starBD+23 3130 ([Fe/H=-2.6). The value was derived from the forbidden line[O I at 630 nm and from six weak Fe II lines, with a S/N ratiosubstantially larger than those obtained before, thanks to theefficiency of the VLT-UVES instrument at Paranal. We obtain[O/Fe=0.71+/-0.25, a value 0.36 dex higher than the value obtained fromthe same lines by Fulbright and Kraft [AJ 118 (1999) 527, but 0.46lower than the one derived by Israelian et al. [ApJ 507 (1998) 805 fromthe UV OH bands.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

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