Estimation of the total masses of star clusters

Details Estimation of the total masses of star clusters Estimation of the total masses of star clusters

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...44d&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, Mar.-Apr. 1988, p. 44-52. In Russian.

Statistics

Computation

Peculiar Stars, Star Clusters, Stellar Mass, Stellar Motions, Computational Astrophysics, Molecular Clouds, Velocity Distribution

Scientific paper

The Naumova-Ogorodnikov (1973) method for estimating the total masses of star clusters is extended to the case when the cluster velocity and the dispersion of peculiar star-field velocities are comparable. The moments of the first and second orders of peculiar velocity variations for field stars in the neighborhoods of clusters are determined. It is concluded that the proposed approach can be used to estimate the total masses and tangential velocities of giant molecular clouds near the sun.

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