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

M. -R. L. Cioni
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Abstract

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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M. -R. L. Cioni. 2006-11-13. Star Formation History across the Magellanic Clouds and other Local Group galaxies. https://arxiv.org/abs/astro-ph/0611389

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