The mass content in the region of the cluster NGC 1750

Details The mass content in the region of the cluster NGC 1750 The mass content in the region of the cluster NGC 1750

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002newa....7..101m&link_type=abstract

New Astronomy, Volume 7, Issue 2, p. 101-106.

Astronomy and Astrophysics

Astronomy

Scientific paper

Kinematical information has been used to solve the Jeans' equation to provide a mass estimate for the open cluster NGC 1750. Using published data we have also applied the Michie-King model to estimate the mass in the cluster. The comparison of these masses gives the best estimation of mass in the region of this cluster as 1.01×104 Msolar, which indicates that the cluster may be a massive cluster. Checks of the density distribution and isotropy of the stellar velocity distribution are given.

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