On the age difference between the oldest Population I and the extreme Population II stars

Astronomy and Astrophysics – Astrophysics

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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

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