activity
20132026
most citedActive Galactic Nuclei Feedback in an Elliptical Galaxy with the Most Updated AGN Physics (I): Low-angular Momentum Case

136 citations · 912 across the 35 of their papers we have counts for

collaborators
Showing 2018Show all

6 papers · 1 filter

astro-ph.HE2018★ 42 cited

Spectral Energy Distribution of the inner accretion flow around Sgr A* -- Clue for a weak outflow in the innermost region

Ren-Yi Ma, Shawn R. Roberts, Ya-Ping Li +1

Sgr A* represents a unique laboratory for the detailed study of accretion processes around a low-luminosity supermassive black hole (SMBH). Recent X-ray observations have allowed f…

astro-ph.HE2018★ 2 cited

Numerical study of active galactic nucleus feedback in an elliptical galaxy with {\it MACER}

Feng Yuan, Jeremiah P. Ostriker, DooSoo Yoon +5

This paper summarizes our recent works of studying AGN feedback in an isolated elliptical galaxy by performing high-resolution hydrodynamical numerical simulations. Bondi radius is…

astro-ph.HE2018★ 29 cited

Reconciling the Quasar Microlensing Disc Size Problem with a Wind Model of Active Galactic Nucleus

Ya-Ping Li, Feng Yuan, Xinyu Dai

Many analyses have concluded that the accretion disc sizes measured from the microlensing variability of quasars are larger than the expectations from the standard thin disc theory…

astro-ph.HE2018★ 41 cited

Active Galactic Nuclei Feedback in an Elliptical Galaxy with the Most Updated AGN Physics (II): High-Angular Momentum Case

Doosoo Yoon, Feng Yuan, Zhao-Ming Gan +3

This is the second paper of our series of works of studying the effects of active galactic nuclei (AGN) feedback on the cosmological evolution of an isolated elliptical galaxy by p…

astro-ph.HE2018★ 40 cited

Stellar and AGN feedback in isolated early-type galaxies: the role in regulating star formation and ISM properties

Ya-Ping Li, Feng Yuan, Houjun Mo +6

Understanding how galaxies maintain the inefficiency of star formation with physically self-consistent models is a central problem for galaxy evolution. Although numerous theoretic…

astro-ph.HE2018★ 3 cited

The Profiles of Fe Kα Line From the Inhomogeneous Accretion Flow

Xiao-Di Yu, Ren-Yi Ma, Ya-Ping Li +2

The clumpy disc, or inhomogeneous accretion flow, has been proposed to explain the properties of accreting black hole systems. However, the observational evidences remain to be exp…