Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-12-05
Astrophys.J.636:L133-L136,2006
Astronomy and Astrophysics
Astrophysics
4 Pages - 3 figures - Accepted for publication in ApJ Letters
Scientific paper
10.1086/500209
We report on the serendipitous discovery of ~ 500 low-mass candidate PMS stars in the vicinity of the stellar association LH 52 in the Large Magellanic Cloud. We present evidence that the red faint sequence of these stars seen in the CMD of LH 52 from HST/WFPC2 observations belongs only to the association and follows almost perfectly isochrone models for PMS stars of masses down to ~ 0.3 M_solar. We find that this feature has a Galactic counterpart and that the mass spectrum of the candidate PMS stars in LH 52 seems to correspond to a Salpeter IMF with a slope Gamma ~ -1.26 in the mass range 0.8 - 1.4 M_solar.
Brandner Wolfgang
Gouliermis Dimitrios
Henning Th
No associations
LandOfFree
The low-mass pre-main sequence population of the stellar association LH 52 in the Large Magellanic Cloud discovered with Hubble Space Telescope WFPC2 Observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The low-mass pre-main sequence population of the stellar association LH 52 in the Large Magellanic Cloud discovered with Hubble Space Telescope WFPC2 Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The low-mass pre-main sequence population of the stellar association LH 52 in the Large Magellanic Cloud discovered with Hubble Space Telescope WFPC2 Observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-86342