The metal abundance and age of the globular cluster Ruprecht 106

Astronomy and Astrophysics – Astronomy

Scientific paper

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Abundance, Chronology, Color-Magnitude Diagram, Globular Clusters, Metallicity, Stellar Spectrophotometry, Calcium, Fine Structure, Galactic Structure, Halos, Hydrogen, Iron

Scientific paper

The metal abundance of the globular cluster Ruprecht 106 was determined spectroscopically, using the 'reddening independent' method described by Armandroff and Da Costa (1991). It was found that the abundance of the Ruprecht cluster equals the value suggested by Buonanno et al. (1990), thereby removing the contradiction with the result of VandenBerg et al. (1990).

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