Black hole evolution: II. Spinning black holes in a supernova-driven turbulent interstellar medium
Supermassive black holes (BH) accrete gas from their surroundings and coalesce with companions during galaxy mergers, and both processes change the BH mass and spin. By means of high-resolution hydrodynamical simulations of galaxies, either idealised or embedded within the cosmic web, we explore th...
| Κύριοι συγγραφείς: | , , , , |
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| Μορφή: | Journal article |
| Έκδοση: |
Oxford University Press
2014
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