Computer Science – Numerical Analysis
Scientific paper
Nov 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....61..391d&link_type=abstract
Astronomy and Astrophysics, vol. 61, no. 3, Nov. 1977, p. 391-396.
Computer Science
Numerical Analysis
12
Astronomical Models, Mathematical Models, Star Clusters, Stellar Motions, Stellar Systems, Monte Carlo Method, Numerical Analysis, Star Distribution, Stellar Evolution
Scientific paper
Two series of analytical models, defined by two-parameter phase density distributions, are presented for the structure of spherical stellar systems. Two of the models can be adjusted to the results of numerical simulations by the Monte Carlo method. The time evolution of the model and scaling parameters obtained in the fit follow a power law. The evolution of the core does not seem to be homologous.
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