Two channels of supermassive black hole growth as seen on the galaxies mass-size plane
We investigate the variation of black hole masses (MBH) as a function of their host galaxy stellar mass (M∗) and half-light radius (Re). We confirm that the scatter in MBH within this plane is essentially the same as that in the MBH–σ relation, as expected from the negligible scatter reported in the...
| Главные авторы: | , , |
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| Формат: | Journal article |
| Опубликовано: |
Oxford University Press
2017
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