Star Formation History across the Magellanic Clouds and other Local Group galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

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5 pages, 3 figures, contributed talk to the workshop "Why galaxies care about AGB stars", Vienna, August 7-11, 2006

Scientific paper

The Ks magnitude distribution of asymptotic giant branch stars provides important constraints on the spatial variation of metallicity and mean-age of the stellar population of galaxies. Here, I present results of the investigation of these parameters across the Magellanic Clouds, M33, NGC 6822 and SagDIG and I discuss the tremendous improvement that new wide-field near-infrared instruments (i.e. VISTA) will provide on our understanding of the global intrinsic as well as dynamical history of these systems.

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