Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations
Massive black hole (MBH) coalescences are powerful sources of low-frequency gravitational waves. To study these events in the cosmological context, we need to trace the large-scale structure and cosmic evolution of a statistical population of galaxies, from dim dwarfs to bright galaxies. To cover su...
| Egile Nagusiak: | , , , , , , , , , , , , , , |
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| Formatua: | Journal article |
| Hizkuntza: | English |
| Argitaratua: |
Oxford University Press
2020
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