The Star Formation History of Nearby Dwarf Galaxies: problems, methods and results
The synthetic color-magnitude diagram (CMD) methodology to study the star formation history (SFH) of nearby galaxies is briefly reviewed. Firstly the most significant features of the CMD for this task are discussed. Then, the procedure of computing synthetic CMDs is explained and the main results obtained by our group in the last few years
Aparicio, A.
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12
1998