Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aj.....99.1961f&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 99, June 1990, p. 1961-1970.
Astronomy and Astrophysics
Astronomy
21
Abundance, Barium, Iron, Red Giant Stars, Metallicity, Peculiar Stars, Spectral Line Width, Stellar Color
Scientific paper
An intermediate-dispersion abundance analysis has been carried out on a sample of 21 barium and 14 comparison stars. The excess of barium over iron has been used as the most representative indicator of peculiarity. These excesses are higher in the peculiar stars than in the nonpeculiar stars. Particularly interesting is the case of HD 67447, included in the comparison stars, with an excess Ba/Fe abundance = 1.61, probably a new barium star. A trend indicating a possible anticorrelation between barium overabundance and metallicity favors the suggestion that the barium strong group is older than the barium weak one.
Cornide Manuel
Fernández-Villacañas José-Luis
Rego M.
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