The star formation history of intermediate redshift late-type galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

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9 pages, 7 figures, uses mn2e.cls. Accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2004.08290.x

We combine the latest observations of disk galaxy photometry and rotation curves at moderate redshift from the FORS Deep Field (FDF) with simple models of chemical enrichment. Our method describes the buildup of the stellar component through infall of gas and allows for gas and metal outflows. In this framework, we keep a minimum number of constraints and we search a large volume of parameter space, looking for the models which best reproduce the photometric observations in the observed redshift range (0.5

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