A new grid of evolutionary synthesis models

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, 1 figure, proceedings of the conference Pathways Through an Eclectic Universe, Eds. T.Mahoney, A. Vazdekis & J. Knape

Scientific paper

We present new evolutionary synthesis models for Single Stellar Populations
covering a wide range in age and metallicity. The most important difference
with existing models is the use of NLTE atmosphere models for the hot stars (O,
B, WR, post-AGB stars, and planetary nebulae) that have an important impact in
the stellar cluster's ionizing spectra.

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