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Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics

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Figure

Figure 1. Density (sound speedPpanel shows a power law approximation for the density profile intop) and velocity (bottom) as a function ofradius for the analytic two temperature solution for three differentvalues of the ionization radius RI, as indicated in
Figure 2. Ionizing luminosity as a function of neutral BondiThe dashed lines correspond to the specific choice ofsound speed and ionization front radius, assuming an inner cut offradiusdensity (top), and as a function of ionization front recombinationtime (b
Figure 4. Relative difference between the simulation and theanalytic solution for the two temperature Bondi accretion withionization and a constant ionization front radius, at the final sim-ulation time t = 40 yr.
Figure 8. Ionization front radius as a function of time for simula-tions with a smooth transition from ionized to neutral region, self-consistent ionization, and a numerically seeded instability
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