Young stellar populations in the Magellanic Clouds
| dc.creator | Vallenari, A. | |
| dc.date | 2007-11-29 | |
| dc.date.accessioned | 2026-07-07T08:46:02Z | |
| dc.date.available | 2026-07-07T08:46:02Z | |
| dc.description | 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 | |
| dc.description | 5 pages, in XXI Century Challenges for Stellar Evolution, in "Memorie della Societa' Astronomica Italiana", Vol. 79 No. 2, eds. S. Cassisi & M. Salaris | |
| dc.identifier | https://arxiv.org/abs/0711.4719 | |
| dc.identifier | http://arxiv.org/abs/0711.4719 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/143151 | |
| dc.subject | Astrophysics | |
| dc.title | Young stellar populations in the Magellanic Clouds | |
| dc.type | text |