Decay dynamics of nonstationary open clusters

Details Decay dynamics of nonstationary open clusters Decay dynamics of nonstationary open clusters

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..704d&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, July-Aug. 1985, p. 704-710) Soviet Astronomy (ISSN 0038-5301), vol. 29, July-Aug. 1985, p. 4

Statistics

Computation

2

Celestial Mechanics, Open Clusters, Stellar Motions, Astronomical Models, Computational Astrophysics, Field Theory (Physics), Stellar Evolution

Scientific paper

Numerical experiments for studying the dynamics of non-isolated open star clusters have been carried out. Mass escape of stars from a non-stationary cluster into the Galaxy's field has been examined. The model of the halo of a cluster which is expanding as a result of the relaxation of the system due to weak stellar encounters was used. Arguments are given in favour of non-stationarity of the open clusters M67 and NGC 188.

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