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The Role of Outflow Feedback on Accretion of Compact Objects in Accretion Disk of Active Galactic Nuclei

  • Authors: Ken Chen, Jia Ren, Zi-Gao Dai

Ken Chen et al 2023 The Astrophysical Journal 948 .

  • Provider: AAS Journals

Caption: Figure 5.

Comparison between the BH accretion timescale and the cavity evolution timescale, and the corresponding reduced BH mass accretion rate. Top rows show t acc/(t cav + t ref) and bottom rows show ﹩{\dot{M}}_{\mathrm{BH},\mathrm{red}}/{\dot{M}}_{\mathrm{Edd}}﹩. Three columns show the s = 0.2, 0.5, and 0.8 cases with m BH = 10M , respectively. In the top-middle panel, the magenta, red, and green lines represent the same boundaries as in Figure 1; the yellow, orange, brown lines, and left regions represent the boundaries of ﹩{r}_{\mathrm{obd}}\leqslant {r}_{\mathrm{tr}}﹩, r obdr rad−gas, and r obdr es−ff, respectively; the cyan line and above region represent the boundary of ﹩{t}_{\mathrm{acc}}\leqslant {t}_{\mathrm{bre}}﹩.

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