Mauro, Francesco; Bidin, Christian Moni; Geisler, D; Saviane, Ivo; Da Costa, Gary; Gormaz-Matamala, A C; Vasquez, S; Chene, A N; Cohen, Roger E.; Dias, B
Context. When they are established with sufficient precision, the ages, metallicities and kinematics of Galactic globular clusters (GGCs) can shed much light on the dynamical and chemical evolution of the Galactic halo and bulge. While the most fundamental way of determining GC abundances is by means of high-resolution spectroscopy, in practice this method is limited to only the brighter stars in the nearest and less reddened objects. This restriction has, over the years, led to the development...[Show more]
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