activity
20132026
most citedHydrodynamical numerical simulation of wind production from black hole hot accretion flows at very large radii

66 citations · 353 across the 36 of their papers we have counts for

collaborators
Showing 2019Show all

5 papers · 1 filter

astro-ph.HE2019★ 7 cited

Magnetohydrodynamic numerical simulation of the outflows driven by magnetic field and radiation force from the corona above a thin disk

Xiao-Hong Yang, De-Fu Bu, Qi-Xiu Li

A hot corona is suggested to be above the standard thin disk. The anisotropy of hard X-ray emission in radio-quiet active galactic nuclei implies that the corona is not static and…

astro-ph.HE2019★ 3 cited

Active galactic nuclei feedback at parsec scale

De-Fu Bu, Xiao-Hong Yang

We perform simulations to study the effects of active galactic nuclei (AGNs) radiation and wind feedback on the properties of slowly rotating accretion flow at parsec scale. We fin…

astro-ph.HE2019★ 6 cited

Hot accretion flow around neutron stars

De-Fu Bu, Er-Lin Qiao, Xiao-Hong Yang

We perform as the first time hydrodynamic simulations to study the properties of hot accretion flow (HAF) around a neutron star (NS). The energy carried by the HAF will eventually…

astro-ph.HE2019★ 8 cited

What is the real accretion rate onto a black hole for low angular momentum accretion?

De-Fu Bu, Xiao-Hong Yang

Mass accretion rate is a key parameter in accretion disk theory. It determines black hole accretion mode. In large scale cosmological simulations studying galaxy formation and evol…

astro-ph.HE2019★ 1 cited

Quenching black hole accretion by active galactic nuclei feedback

De-Fu Bu, Xiao-Hong Yang

Observations of many dim galactic nuclei in local universe give good estimation of gas density and temperature at Bondi radius. If we assume the black hole accretes at Bondi accret…