Article ID Journal Published Year Pages File Type
1778725 New Astronomy 2016 6 Pages PDF
Abstract

•Fundamental parameters are determined.•Apex coordinates for NGC 188 are calculated.•Kinematical parameters of the clusters are derived.

In this paper, we present our results for the photometric and kinematical studies of old open cluster NGC 188. We determined various astrophysical parameters like limited radius, core and tidal radii, distance, luminosity and mass functions, total mass, relaxation time etc. for the cluster using 2MASS catalog. We obtained the cluster’s distance from the Sun as 1721 ± 41 pc and log (age)= 9.85 ± 0.05 at Solar metallicity. The relaxation time of the cluster is smaller than the estimated cluster age which suggests that the cluster is dynamically relaxed. Our results agree with the values mentioned in the literature. We also determined the clusters apex coordinates as (281°.88, −44∘−44∘.76) using AD-diagram method. Other kinematical parameters like space velocity components, cluster center and elements of Solar motion etc. have also been computed.

Related Topics
Physical Sciences and Engineering Physics and Astronomy Astronomy and Astrophysics
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