Resolved and unresolved populations: statistics and synthesis models
Astrophysics
2007-05-23 v1
Abstract
In this contribution, I present the 90% confidence limits on the diagnostic diagrams of EW(WR bump) and L(WR bump)/L(Hb) ratio vs. EW(Hb) resulting from evolutionary synthesis models that include the statistical dispersion due to finite stellar populations in real star forming regions.
Cite
@article{arxiv.astro-ph/0206169,
title = {Resolved and unresolved populations: statistics and synthesis models},
author = {M. Cervino},
journal= {arXiv preprint arXiv:astro-ph/0206169},
year = {2007}
}
Comments
2 pages, 2 figures, To be presented in IAU Symp. 212