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Bridging Scales in Black Hole Accretion and Feedback: Studying Supermassive Black Holes
Manage episode 417533461 series 3474373
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This story was originally published on HackerNoon at: https://hackernoon.com/bridging-scales-in-black-hole-accretion-and-feedback-studying-supermassive-black-holes.
The details of how gas flows into the galactic nucleus from large cosmic distances and how the SMBH in turn imparts feedback into the galaxy remain unresolved.
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Most nearby galaxies are found to harbor central supermassive black holes (SMBHs) whose masses are correlated with properties of the stellar components of their hosts (e.g., Magorrian et al. 1998; Ferrarese & Merritt 2000; Gebhardt et al. 2000; Kormendy & Ho 2013). However, the details of how gas flows into the galactic nucleus from large cosmic distances and how the SMBH in turn imparts feedback into the galaxy remain coupled unresolved problems.
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