A new grid of evolutionary synthesis models
Astrophysics
2007-11-21 v1
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.
Cite
@article{arxiv.0711.3141,
title = {A new grid of evolutionary synthesis models},
author = {M. Mollá and M. L. García-Vargas and Alessandro Bressan and Pedro Gómez-Alvarez},
journal= {arXiv preprint arXiv:0711.3141},
year = {2007}
}
Comments
2 pages, 1 figure, proceedings of the conference Pathways Through an Eclectic Universe, Eds. T.Mahoney, A. Vazdekis & J. Knapen, Tenerife 2007