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摘要
This paper, the second in a series on radiation-regulated accretion onto black holes (BHs) from galactic scales, focuses on the effects of radiation pressure and angular momentum of the accreting gas. We simulate accretion onto intermediate-mass black holes, but we derive general scaling relationships that are solutions of the Bondi problem with radiation feedback valid for any mass of the BH M-bh. Thermal pressure of the ionized sphere around the BH regulates the accretion rate, producing periodic and short-lived luminosity bursts. We find that for ambient gas densities exceeding n(H,infinity)(cr) alpha M-bh(-1), the period of the oscillations decreases rapidly and the duty cycle increases from 6%, in agreement with observations of the fraction of active galactic nuclei at z similar to 3, to 50%. The mean accretion rate becomes Eddington limited for n(H,infinity) > n(H,infinity)(Edd) similar or equal to n(H,infinity)(cr)T(infinity,4)(-1) where T-infinity,T-4 is the gas temperature in units of 10(4) K. In the sub-Eddington regime, the mean accretion rate onto BHs is about 1% T-infinity,4(2.5) of the Bondi rate, and thus is proportional to the thermal pressure of the ambient medium. The period of the oscillations coincides with the depletion timescale of the gas inside the ionized bubble surrounding the BH. Gas depletion is dominated by a pressure gradient pushing the gas outward if n(H,infinity) < n(H,infinity)(cr) and by accretion onto the BH otherwise. Generally, for n(H,infinity) < n(H,infinity)(cr) angular momentum does not significantly affect the accretion rate and period of the oscillations.
- 出版日期2012-3-1
