Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...217..281s&link_type=abstract
Astrophysical Journal, Part 1, vol. 217, Oct. 1, 1977, p. 281-286.
Astronomy and Astrophysics
Astronomy
56
Black Holes (Astronomy), Galactic Evolution, Globular Clusters, Stellar Motions, Astronomical Models, Gravitational Collapse, Stellar Mass, Tides, X Ray Stars
Scientific paper
A homological model is employed to follow the dynamical evolution of a globular cluster core containing a massive black hole at its center. Energy is supplied to the core via the inward drift and tidal disruption of stars in the cusp. This outward flow of energy inevitably halts and reverses core collapse. Re-expansion and complete dissolution is the ultimate fate of star clusters in the Galaxy whether they form tight binaries or massive black holes at their centers following catastrophic core collapse. Possible observational consequences of these results are briefly explored.
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