Numerical developments on the dynamical evolution of clusters with more stellar populations

Details Numerical developments on the dynamical evolution of clusters with more stellar populations Numerical developments on the dynamical evolution of clusters with more stellar populations

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mmsai..47..245a&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 47, June 1976, p. 245-254. Research supported by the Consiglio Nazionale delle Rice

Astronomy and Astrophysics

Astrophysics

11

Astrophysics, Fluid Dynamics, Star Clusters, Computer Programs, Convergence, Fokker-Planck Equation, Numerical Integration, Star Distribution, Velocity Distribution

Scientific paper

Moment equations are extended from one to more stellar populations within the framework of the Larson (1970) fluid dynamics approach. Each population is described by its own set of equations with appropriate collision terms. These terms contain quantities pertinent to all the other populations. The full set of equations is integrated simultaneously by computer. The computer program is optimized with respect to convergence speed.

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