Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..47..151s&link_type=abstract
Astrophysics and Space Science, vol. 47, Mar. 1977, p. 151-162.
Astronomy and Astrophysics
Astrophysics
12
Galactic Evolution, Hertzsprung-Russell Diagram, Stellar Evolution, Stellar Models, Astronomical Models, Chemical Evolution, Globular Clusters, Star Clusters, Star Distribution
Scientific paper
The age difference between the oldest Population I stars and the extreme Population II stars is investigated by comparison of observational H-R diagrams with theoretical results using the common input physics and computer program for both Populations. Chemical compositions adopted for Population I and II stars are, X=O.7 and Z=O.02, and X=O.7 and Z= 2 x i0~, respectively. Evidence collected indicates that the open cluster NGC 188 and the globular cluster M92 are the representative samples of the oldest Population I and extreme Population II stars, respectively. Comparison between the observed H-R diagrams and theoretical isochrones in terms of the luminosity of the subgiant region and the turnoff point for NGC 188 and M92, respectively, then suggests that there is a significant age difference between Population I and II objects. The uncertainty of the oxygen abundance in the extreme Population II stars and its effect on their age determination is briefly discussed
Saio Hideyuki
Shibata Yu.
Simoda Mahiro
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