Der Einfluß eines Sterndichtegradienten auf die Verteilung des Gravitations-Mikrofeldes in Sternhaufen

Details Der Einfluß eines Sterndichtegradienten auf die Verteilung des Gravitations-Mikrofeldes in Sternhaufen Der Einfluß eines Sterndichtegradienten auf die Verteilung des Gravitations-Mikrofeldes in Sternhaufen

Oct 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968zphy..212..449b&link_type=abstract

Zeitschrift für Physik, Volume 212, Issue 5, pp.449-457

Mathematics

Probability

Scientific paper

The probability distribution of the gravitational microfield at a fixed space point in a stellar cluster is determined using the Markov-method and neglecting statistical correlations between individual stars so that they are moving independently of each other in the macroscopical field of the whole cluster. In presence of a stellar density gradient, the distribution of the deviations from the mean gravitational field is found to be an anisotropically deformed Holtsmarkian with its maximum shifted to a field deviation vector antiparallel to the density gradient.

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