Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-05-19
Astrophys.J.649:243-247,2006
Astronomy and Astrophysics
Astrophysics
16 pages, 4 figures, accepted for pubblication on ApJ
Scientific paper
10.1086/506013
We present an empirical method to derive photometric metallicity, reddening and distance to old stellar populations by using a few major features of the Red Giant Branch (RGB) in near IR color magnitude diagrams. We combine the observed RGB features with a set of equations linking the global metallicity [M/H] to suitable RGB parameters (colors, magnitudes and slope), as calibrated from a homogeneous sample of Galactic Globular Clusters with different metallicities. This technique can be applied to efficiently derive the main population parameters of old stellar systems, in the view of using ground-based adaptive optics and space facilities to probe the stellar content of remote galaxies.
Ferraro Francesco R.
Origlia Livia
Valenti Elena
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