Abstract
The hydrodynamic formation of massive black holes (BHs) in globular clusters is studied. By incorporating the realistic chemical evolution of globular clusters into the radiation drag model, we scrutinize whether our scenario is successful.
Cite
CITATION STYLE
APA
Kawakatu, N., & Umemura, M. (2004). Formation of massive black holes in globular clusters. Progress of Theoretical Physics Supplement, 155, 355–356. https://doi.org/10.1143/PTPS.155.355
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