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A Hubble View of Star Forming Regions in the Magellanic Clouds

The Magellanic Clouds (MCs) offer an outstanding variety of young stellar associations, in which large samples of low-mass stars (with masses less than 1 solar mass) currently in the act of formation can be resolved and explored sufficiently with the Hubble Space Telescope. These pre-main sequence (PMS) stars provide a unique snapshot of the star formation process, as it is being recorded for the last 20 Myr, and they give important information on the low-mass Initial Mass Function (IMF) of their host environments. We present the latest results from observations with the Advanced Camera for Surveys (ACS) of such star-forming regions in the MCs, and discuss the importance of Hubble}for a comprehensive collection of substantial information on the most recent low-mass star formation and the low-mass IMF in the MCs.

preprint2007arXivOpen access
D. A. GouliermisTh. HenningW. BrandnerM. R. RosaA. E. DolphinM. SchmalzlE. HennekemperH. ZinneckerN. PanagiaY. -H. ChuB. BrandlS. P. QuanzM. RobbertoG. de MarchiR. A. GruendlM. Romaniello
astro-ph
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D. A. GouliermisTh. HenningW. BrandnerM. R. RosaA. E. DolphinM. SchmalzlE. HennekemperH. ZinneckerN. PanagiaY. -H. ChuB. BrandlS. P. QuanzM. RobbertoG. de MarchiR. A. GruendlM. Romaniello

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