Multiple stellar populations in Magellanic Cloud clusters. II. Evidence also in the young NGC 1844?
We used Hubble Space Telescope observations to study the young cluster NGC 1844 in the Large Magellanic Cloud (LMC). We estimated the fraction and the mass-ratio distribution of photometric binaries and report that the main sequence presents an intrinsic breadth which cannot be explained only in terms of photometric errors, and is unlikely because
Milone, A. P. et al.
Fecha de publicación:
7
2013