The Motion of Halo Stars in Dynamical Numerical Models of Open Clusters

Details The Motion of Halo Stars in Dynamical Numerical Models of Open Clusters The Motion of Halo Stars in Dynamical Numerical Models of Open Clusters

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005arep...49..604d&link_type=abstract

Astronomy Reports, vol. 49, Issue 8, p.604-610

Astronomy and Astrophysics

Astronomy

Scientific paper

Equations of motion containing a small parameter μ are derived for stars at the peripheries of open star clusters. The parameter μ is obtained for six numerical open-cluster models. The general analytical solution of these equations of motion for μ = 0 is found. An iterative method is used to derive the frequencies of the stellar motions for first-order expansions in μ of the solutions of the equations of motion for stars at the cluster periphery. Applications of the results are discussed.

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