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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 7.

Comparison between the NS accretion timescale and the cavity evolution timescale, and the corresponding reduced NS mass accretion rate. The top rows show t acc/(t cav + t ref) and the bottom rows show ﹩{\dot{M}}_{\mathrm{NS},\mathrm{red}}/{\dot{M}}_{\mathrm{Edd}}﹩. The three columns show the cases of m NS = 1.4M and s = 0.5, with B = 1012 G, B = 109 G, treated as a BH, respectively. The case treated as a BH means that the NS is set to behave as a BH without the hard surface and magnetic field, and the only energy source is the circum-NS disk.

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