arXiv · 0711.3141
A new grid of evolutionary synthesis models
Abstract
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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M. Mollá, M. L. García-Vargas, Alessandro Bressan, Pedro Gómez-Alvarez. 2007-11-20. A new grid of evolutionary synthesis models. https://arxiv.org/abs/0711.3141
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