Article citations

    T. M. Girard, W. M. Grundy, C. E. L pez and W. F. van Altena, “Relative Proper Motions and the Stellar Velocity Dispersion of the Open Cluster M67,” Astron. J., Vol. 98, No. 1, 1989, pp. 227-243. doi:10.1086/115139

has been cited by the following article:

  • TITLE: Examining the M67 Classification as an Open Cluster
  • AUTHORS: Shimmon Naim, Evgeny Griv
  • KEYWORDS: Photometers; Techniques; Photometric; Open Clusters and Associations; M67; Galaxies; Star Clusters
  • JOURNAL NAME: International Journal of Astronomy and Astrophysics DOI: 10.4236/ijaa.2012.23020 Sep 05, 2014
  • ABSTRACT: The cluster M67 (= NGC 2682) in Cancer is a rich stellar cluster, usually classified as an open cluster. Using our own observations with the 0.4 m telescope, we show that M67 is a tight group of about 1200 stars. The actual radius of the cluster is about 3.1 pc and the average mass of a star in the system is about . We also show that the ratio of the mean kinetic energy of the cluster to its mean gravitational potential energy , while the value predicted by the virial theorem is equal to . So the system is a gravitationally bound. This value of is considered as an evidence of quasi-stability of the cluster and allows us to use the Chandrasekhar-Spitzer relaxation time for M67 Myr as a characteristic dynamical relaxation time of the system. As the cluster is almost twice older its half-life time , it is argued that M67 was in the past (about 4 Gyr ago, close to its forma-tion) a relatively small ( stars) globular cluster, but got “open cluster” shape due to the dynamical evapora-tion of the majority of its stars.