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Fig. 3

image

Adiabatic accretion with erot = 0.3: evolution of the mass-weighted electron density (top; neρ/ 1.93 × 10-24 cm-3) and temperature (bottom) radial profiles, sampled every 1 Myr (from dark blue to cyan). The cuspy profiles are similar to the classic Bondi solution (G13), smoothly joining the galactic gradients at large r.

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