The maximum spherical accretion rate onto a central black hole in a Hernquist galaxy increases with the galaxy's characteristic linear density and decreases with radiation, approaching the classical Bondi rate when the outer boundary is far beyond the semi-Bondi radius.
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Bondi accretion in the finite luminous region of elliptical galaxies
The maximum spherical accretion rate onto a central black hole in a Hernquist galaxy increases with the galaxy's characteristic linear density and decreases with radiation, approaching the classical Bondi rate when the outer boundary is far beyond the semi-Bondi radius.