Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aj....100..445v&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 100, Aug. 1990, p. 445-468.
Astronomy and Astrophysics
Astronomy
306
Color-Magnitude Diagram, Globular Clusters, Metallic Stars, Metallicity, Stellar Composition, Astronomical Photometry, Chemical Composition, Interstellar Extinction, Star Clusters, Statistical Analysis, Stellar Evolution
Scientific paper
A color-difference technique for estimating the relative ages of globular clusters with similar chemical compositions on the basis of their CM diagrams is described and demonstrated. The theoretical basis and implementation of the procedure are explained, and results for groups of globular clusters with m/H = about -2, -1.6, and -1.3, and for two special cases (Palomar 12 and NGC 5139) are presented in extensive tables and graphs and discussed in detail. It is found that the more metal-deficient globular clusters are nearly coeval (differences less than 0.5 Gyr), whereas the most metal-rich globular clusters exhibit significant age differences (about 2 Gyr). This result is shown to contradict Galactic evolution models postulating halo collapse in less than a few times 100 Myr.
Bolte Michael
Stetson Peter B.
VandenBerg Don. A.
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