MODELING STELLAR POPULATIONS NEAR AND FAR
I summarize the current status of the determinations of galaxy masses based on population synthesis models at ages at which the TP-AGB stars dominate the NIR luminosity (=1 Gyr). Mass estimates of galaxies with dominant stellar populations in this age range thus depend critically on the treatment of...
Guardado en:
| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2011
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| Materias: | |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57121297013 |
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