A new grid of evolutionary synthesis models

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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.
2 pages, 1 figure, proceedings of the conference Pathways Through an Eclectic Universe, Eds. T.Mahoney, A. Vazdekis & J. Knapen, Tenerife 2007

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/142511

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0711.3141
 http://arxiv.org/abs/0711.3141

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arXiv