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.
This paper is available on Arxiv under CC 4.0 license. Authors: Hyerin Cho , Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA and Black Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USA; Ben S.
Most nearby galaxies are found to harbor central supermassive black holes whose masses are correlated with properties of the stellar components of their hosts . 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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