Synthetic Stellar Clusters for Pop III

Details Synthetic Stellar Clusters for Pop III Synthetic Stellar Clusters for Pop III

1999-12-22

arxiv.org/abs/astro-ph/9912472v1

Astronomy and Astrophysics

Astrophysics

2 pages, incl. 2 figures, "The First Stars", Proceedings of the second MPA/ESO workshop, Eds.: Weiss, Abel, Hill, Springer, He

Scientific paper

10.1007/10719504_23

We present preliminary results of an incoming theoretical work concerning the integrated properties of the Population III clusters of stars. On the basis of synthetic Color-Magnitude Diagrams, we provide a grid of optical and near-IR colors of Simple Stellar Populations with very low metallicity (Z=10$^{-10}$ and Z=10$^{-6}$) and age which spans from 10 Myr to 15 Gyr. A comparison with higher metallicities up to 0.006 is also shown, disclosing sizable differences in the CMD morphology, integrated colors and Spectral Energy Distribution (SED).

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