Abundance determinations from low-dispersion spectra of globular-cluster stars

Details Abundance determinations from low-dispersion spectra of globular-cluster stars Abundance determinations from low-dispersion spectra of globular-cluster stars

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..518b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, July 1984, p. 518-529.

Astronomy and Astrophysics

Astronomy

18

Globular Clusters, Stellar Composition, Stellar Spectra, Spectrum Analysis, Stellar Models

Scientific paper

A number of synthetic spectra have been computed for comparison with Canterna, Harris, and Ferrall's low-dispersion spectra of stars in the globular clusters 47 Tuc, NGC 288, NGC 362, M15, M2, and Pal 12. Spectral indices have been deduced from the synthetic spectra and compared with the observed indices. The mean abundances of these six clusters are deduced.

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