Abundances of elements of the Fe-group in metal-poor stars

Details Abundances of elements of the Fe-group in metal-poor stars Abundances of elements of the Fe-group in metal-poor stars

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...241..501g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 241, no. 2, Jan. 1991, p. 501-525.

Physics

194

Iron, Metallicity, Stellar Composition, Stellar Physics, Globular Clusters, Nuclear Fusion, Spectral Line Width, Stellar Atmospheres, Stellar Spectra

Scientific paper

The paper presents results of an analysis of the abundances of elements of the Fe group and Si in 19 field stars with Fe/H ranging from -2.7 to -0.2. The hyperfine structure is fully considered for lines of the odd elements. The abundances in metal-poor stars are compared with the predictions of nucleosynthesis theories for Fe group elements. A promising agreement with recent calculations for production of these elements by type II SNe is obtained.

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