Population synthesis at short wavelengths and spectrophotometric diagnostic tools for galaxy evolution
Astrophysics
2007-09-19 v1
Abstract
Taking advantage of recent important advances in the calculation of high-resolution spectral grids of stellar atmospheres at short wavelengths, and their implementation for population synthesis models, we briefly review here some special properties of ultraviolet emission in SSPs, and discuss their potential applications for identifying and tuning up effective diagnostic tools to probe distinctive evolutionary properties of early-type galaxies and other evolved stellar systems.
Cite
@article{arxiv.0709.2711,
title = {Population synthesis at short wavelengths and spectrophotometric diagnostic tools for galaxy evolution},
author = {A. Buzzoni and E. Bertone and M. Chavez and L. H. Rodriguez-Merino},
journal= {arXiv preprint arXiv:0709.2711},
year = {2007}
}
Comments
Invited contribution to "New quests in stellar astrophysics. II: Ultraviolet properties of evolved stellar populations" (Puerto Vallarta, Mexico, Apr 2007), eds. M. Chavez et al. - More info on the UVBLUE spectral library at http://www.bo.astro.it/~eps/home.html