PAL 1. The Youngest Globular Cluster or the Oldest Open Cluster?
We present a color magnitude diagram (CMD) in the V and I bands reaching 4 magnitudes below the turn off (TO) and intermediate resolution spectra for 4 giant branch (GB) stars. The spectra allowed us to determine the cluster metallicity and radial velocity for the cluster Pal 1. The metallicity has been determined using the CaII triplet and other
Rosenberg, A. et al.
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1997