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Computing models of the chemical and spectro-photometric
evolution of galaxies and constrain them with the history
told by the fossils
we can find in the nearby universe
(Milky Way, Spirals,
Low Surface Brightness galaxies)
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Using ultra-violet to infrared data to study
extinction and star formation rate in nearby
late-type galaxies (using specially the results of the GALEX mission)
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Using large samples of galaxies to obtain clues
of their evolution, e.g. studying
the properties of intermediate redshift
galaxies in the HST
WFPC2 Associations.
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