Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-03-20
Astronomy and Astrophysics
Astrophysics
5 pages, 6 Postscript figures, accepted by MNRAS
Scientific paper
10.1046/j.1365-8711.2002.05508.x
By relying on recently improved Hipparcos parallaxes for the Hyades, Pleiades and Ursa Major clusters we find that stellar models with updated physical inputs nicely reproduce the location in the color magnitude diagram of main sequence stars of different metallicities. Stars in the helium burning phase are also discussed, showing that the luminosity of giants in the Hyades, Praesepe and Ursa Major clusters appears to be in reasonable agreement with theoretical predictions. A short discussion concerning the current evolutionary scenarios closes the paper.
Castellani Vittorio
Degl'Innocenti Scilla
Prada Moroni Pier Giorgio
Tordiglione V.
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