Young stellar populations in the Magellanic Clouds .
DOI: 10.48550/arXiv.0711.4719
Bibcode: 2008MmSAI..79..448V
Vallenari, A.
Italy
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. 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 105 yrs to several Myr ago
2008
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Memorie della Societa Astronomica Italiana
eHST
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