Relative abundance determinations in extremely metal poor giants. II - Transition probabilities and the abundance determinations

Details Relative abundance determinations in extremely metal poor giants. II - Transition probabilities and the abundance determinations Relative abundance determinations in extremely metal poor giants. II - Transition probabilities and the abundance determinations

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...350..173p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 350, Feb. 10, 1990, p. 173-185.

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94

Giant Stars, Metallicity, Stellar Composition, Transition Probabilities, Abundance, Globular Clusters, Iron

Scientific paper

The abundances of Fe and other elements are determined for a star of intermediate metallicity and for nine extremely metal poor stars, including two members of the globular cluster M92 and CD -38 deg 245. The accuracy of the transition probabilities for Fe I and other elements is evaluated. The distribution of the abundances of other elements with respect to Fe is the same for most of the cases studied. Manganese is the only element that shows a different relative abundance in an extremely metal poor star.

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