Black holes and core expansion in massive star clusters
In this study we present the results from realistic N-body modelling of massive star clusters in the Magellanic Clouds. We have computed eight simulations with N ∼ 105 particles; six of these were evolved for at least a Hubble time. The aim of this mode
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Mackey_Black_holes_and_core_expansion_2008.pdf||1.34 MB||Adobe PDF||Request a copy|
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