Homogeneous metallicities and radial velocities for Galactic globular clusters: First CaT metallicities for twenty clusters
Well determined radial velocities and abundances are essential for analyzing the properties of the globular cluster system of the Milky Way. However more than 50% of these clusters have no spectroscopic measure of their metallicity. In this context, this
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|Source:||Astronomy and Astrophysics|
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