Evolution of dense rotating star clusters in the cores of early galaxies

Details Evolution of dense rotating star clusters in the cores of early galaxies Evolution of dense rotating star clusters in the cores of early galaxies

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...18911105g&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #111.05; Bulletin of the American Astronomical Society, Vol. 28, p.1423

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present simulations of the evolution of dense star clusters integrated using a two-dimensional Fokker-Planck approach. Effects of initial rotation, ellipticity, and stellar mergers are included. When an instability criterion is satisfied (Trot/|W| > alpha , where alpha is the stability parameter), a non-axisymmetric component of the potential is applied to model the formation of a stellar bar. Results are interpreted with a view to describing the formation of a massive ( ~ 10(3) M_sun) object near the cluster center which could evolve into the seed black hole of an AGN or quasar.

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