Numerical estimates of the accretion rate on to intermediate-mass black holes
The existence of intermediate-mass (̃103M⊙) black holes (IMBHs) in the centre of globular clusters has been suggested by different observations. The X-ray sources observed in NGC 6388 and in G1 in M31 could be interpreted as being powered by the accretion of matter on to such objects. In this work,...
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| Autores principales: | Pepe, C., Pellizza, L.J. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v430_n4_p2789_Pepe |
| Aporte de: |
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