Metal abundances of RR Lyrae stars - Results from Delta-S spectroscopy

Details Metal abundances of RR Lyrae stars - Results from Delta-S spectroscopy Metal abundances of RR Lyrae stars - Results from Delta-S spectroscopy

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..505s&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, July 1984, p. 505-517.

Astronomy and Astrophysics

Astronomy

12

Cepheid Variables, Metallicity, Stellar Composition, Stellar Spectra, Calibrating, Globular Clusters, Magellanic Clouds, Milky Way Galaxy, Stellar Evolution

Scientific paper

The ΔS method is a means of determining the metal abundances of RR Lyrae stars and related variable stars from low-resolution spectroscopy. This approach has been applied to the measurement of metallicities of field and cluster stars in the Galaxy and in the Magellanic Clouds. This paper reviews the ΔS method, discusses its results and comments on some prospects for future work.

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