Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....98.1624s&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 98, Nov. 1989, p. 1624-1633.
Astronomy and Astrophysics
Astronomy
82
Chronology, Galactic Clusters, Galactic Evolution, Globular Clusters, Milky Way Galaxy, Astronomical Models, Horizontal Branch Stars, Luminosity
Scientific paper
The ages of the Galactic globular clusters are studied, based on a new interpretation of the observed Delta(V) and Fe/H abundance ratio values in terms of a parameterized model. The derived ages are in excellent agreement with those derived from isochrone fitting. Evidence is presented for an age spread of 5 Gyr, suggesting a prolonged epoch of globular cluster formation. It is found that younger clusters have high metallicity. The results suggest that the variations in age describe the observed variation in horizontal-branch morphology in Galactic clusters at a given metallicity.
King Christopher R.
Sarajedini Ata
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