Star Formation Histories from Spectra: What Can We Believe?

Bibcode
2011EAS....48...87K
DOI
10.1051/eas/1148021
Koleva, M.; Cenarro, A. J.; de La Rosa, I.; Sanchez-Blazquez, P.; Vazdekis, A.
Referencia bibliográfica

EAS Publications Series, Volume 48, 2011, pp.87-89

Fecha de publicación:
7
2011
Número de autores
5
Número de autores del IAC
3
Número de citas
0
Número de citas referidas
0
Descripción
To determine the star formation histories of dwarf galaxies we use fossil methods. Compared to the color-magnitude diagrams analyzes, which are well tested and widely accepted, the studies of integrated spectra are still young. In order to assess their capabilities and limitations, we compare the results of three publicly available star formation recovery programs (StarLight, STECKMAP and ULySS).
Tipo
Sin árbitro

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