activity
20082026
most citedThe Radiative Efficiency of Hot Accretion Flows

187 citations · 1.4k across the 50 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2020★ 9 cited

Resolving the Nuclear Radio Emission from M32 with Very Large Array

Sijia Peng, Zhiyuan Li, Loránt O. Sjouwerman +3

The Local Group dwarf elliptical galaxy M32 hosts one of the nearest and most under-luminous super-massive black holes (SMBHs) ever known, offering a rare opportunity to study the…

astro-ph.GA2019★ 1 cited

X-ray spectral shape variations in changing-look Seyfert galaxy SDSSJ155258+273728

Yanli Ai, Liming Dou, Chenwei Yang +7

We analyze the X-ray, optical, and mid-infrared data of a "changing-look" Seyfert galaxy \sdssj15 at . Over a period of one decade (2009 - 2018), its broad H line…

astro-ph.GA2018★ 8 cited

The Bending Feature of the Fermi Bubbles: A Presumed Horizontal Galactic Wind and Its Implication on the Bubbles' Age

Guobin Mou, Dongze Sun, Fuguo Xie

There are two spectacular structures in our Milky Way: the {\it Fermi} bubbles in gamma-ray observations and the North Polar Spur (NPS) structure in X-ray observations. Because of…

astro-ph.GA2018★ 34 cited

NuSTAR Hard X-ray View of Low-luminosity Active Galactic Nuclei: High-energy Cutoff and Truncated Thin Disk

George Younes, Andrew Ptak, Luis C. Ho +5

We report the analysis of simultaneous XMM-Newton+NuSTAR observations of two low-luminosity Active Galactic Nuclei (LLAGN), NGC 3998 and NGC 4579. We do not detect any significant…

astro-ph.GA2017★ 10 cited

Low-mass Active Galactic Nuclei on the Fundamental Plane of Black Hole Activity

Lei Qian, Xiao-Bo Dong, Fu-Guo Xie +2

It is widely known that in active galactic nuclei (AGNs) and black hole X-ray binaries (BHXBs), there is a tight correlation among their radio luminosity (), X-ray luminosity…

astro-ph.GA2013★ 5 cited

Triggering star formation by both radiative and mechanical active galactic nucleus feedback

Chao Liu, Zhao-ming Gan, Fu-guo Xie

We perform two dimensional hydrodynamic numerical simulations to study the positive active galactic nucleus feedback which triggers, rather than suppresses, star formation. Recentl…