A Hubble View of Star Forming Regions in the Magellanic Clouds
D. A. Gouliermis, Th. Henning, W. Brandner, M. R. Rosa, A. E. Dolphin,, M. Schmalzl, E. Hennekemper, H. Zinnecker, N. Panagia, Y.-H. Chu, B. Brandl,, S. P. Quanz, M. Robberto, G. De Marchi, R. A. Gruendl, M. Romaniello
TL;DR
This paper utilizes Hubble Space Telescope observations to study young, low-mass star-forming regions in the Magellanic Clouds, providing insights into recent star formation processes and the initial mass function.
Contribution
It presents new high-resolution observations of star-forming regions in the Magellanic Clouds, enhancing understanding of low-mass star formation and the initial mass function in these environments.
Findings
Resolved low-mass pre-main sequence stars in the MCs
Provided new data on the low-mass IMF in the MCs
Enhanced understanding of recent star formation history
Abstract
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.