Dynamical effects of primordial binaries in star clusters. I - Equal masses

Details Dynamical effects of primordial binaries in star clusters. I - Equal masses Dynamical effects of primordial binaries in star clusters. I - Equal masses

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.257..513h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 257, no. 3, Aug. 1, 1992, p. 513-536. Research supporte

Astronomy and Astrophysics

Astronomy

80

Binary Stars, Globular Clusters, Many Body Problem, Stellar Evolution, Stellar Mass, Celestial Mechanics, Star Clusters, Stellar Models

Scientific paper

The evolution is described of an idealized star cluster in which all stars have the same mass and initially a modest fraction of the stars form hard binaries. The treatment ranges from simple theory based on considerations of time-scales and energetics, through continuum models which include the effects of segregation of binaries, to N-body simulations of systems with a few thousand stars. Particular consideration is given to the circumstances at the close of core collapse and its immediate aftermath.

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