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arXiv · 0711.4719

Young stellar populations in the Magellanic Clouds

Abstract

We discuss the young population of stars and clusters in the Magellanic Clouds. We present the discovery of pre-main sequence candidates in the nebula N~11 in the Large Magellanic Clouds using HST ACS photometry. The comparison of the Colour-Magnitude diagram with pre-main sequence tracks and the presence of Spitzer objects YSO I and II suggest that the star formation has been active for a long period in the region, from a few $10^5$ yrs to several Myr ago

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A. Vallenari. 2007-11-29. Young stellar populations in the Magellanic Clouds. https://arxiv.org/abs/0711.4719

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