Outflows from inflows: the nature of Bondi-like accretion

21 Oct 2019 Waters Tim Aykutalp Aycin Proga Daniel Johnson Jarrett Li Hui Smidt Joseph

The classic Bondi solution remains a common starting point both for studying black hole growth across cosmic time in cosmological simulations and for smaller scale simulations of AGN feedback. In nature, however, there will be inhomogenous distributions of rotational velocity and density along the outer radius ($R_o$) marking the sphere of influence of a black hole... (read more)

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  • ASTROPHYSICS OF GALAXIES
  • HIGH ENERGY ASTROPHYSICAL PHENOMENA