The astrophysical behavior of open clusters along the Milky Way Galaxy

The main aim of this paper is to study the astrophysical behaviour of open clusters’ properties along the Milky Way Galaxy. Near-IR JHKSJHKS (2MASS) photometry has been used for getting a homogeneous Catalog of 263 open clusters’ parameters, which are randomly selected and studied by the author through the last five years; most of them were studied for the first time. The correlations between the astrophysical parameters of these clusters have been achieved by morphological way and compared with the most recent works.