http://arxiv.org/abs/1403.0621
The main aim of this paper is to study the astrophysical behavior of open clusters’ properties along the Milky Way Galaxy. Near-IR {\it JHK$_{S}$} {\it (2MASS)} photometry has been used for getting a homogeneous Catalog of 264 open clusters’ parameters, which are studied for the first time by the author through the last five years. The correlations between the astrophysical parameters of these clusters have been achieved in morphological way and compared with the most recent works.
Tadross. and A. L
Wed, 5 Mar 14
19/75