scholarly journals A Limit Relation between Black Hole Mass and H Width: Testing Super-Eddington Accretion in Active Galactic Nuclei

2003 ◽  
Vol 125 (6) ◽  
pp. 2859-2864 ◽  
Author(s):  
Jian-Min Wang

2020 ◽  
Vol 901 (1) ◽  
pp. 35
Author(s):  
Huynh Anh N. Le ◽  
Jong-Hak Woo ◽  
Yongquan Xue








2006 ◽  
Vol 637 (2) ◽  
pp. 669-681 ◽  
Author(s):  
Yi Liu ◽  
Dong Rong Jiang ◽  
Min Feng Gu


2010 ◽  
Vol 724 (1) ◽  
pp. 386-399 ◽  
Author(s):  
Dohyeong Kim ◽  
Myungshin Im ◽  
Minjin Kim


2012 ◽  
Vol 8 (S290) ◽  
pp. 37-40
Author(s):  
O. González-Martín ◽  
S. Vaughan

AbstractWe have performed a uniform analysis of the power spectrum densities (PSDs) of 104 nearby (z<0.4) active galactic nuclei (AGN) using 209 XMM-Newton/pn observations, including several AGN classes. These PSDs span ≃ 3 decades in temporal frequencies, ranging from minutes to days. We have fitted each PSD to two models: (1) a single power-law model and (2) a bending power-law model. A fraction of 72% show significant variability. The PSD of the majority of the variable AGN was well described by a simple power-law with a mean index of α = 2.01±0.01. In 15 sources we found that the bending power law model was preferred with a mean slope of α = 3.08±0.04 and a mean bend frequency of 〈νb〉 ≃ 2 × 10−4 Hz. Only KUG 1031+398 (RE J1034+396) shows evidence for quasi-periodic oscillations. The ‘fundamental plane’ relating variability timescale, black hole mass, and luminosity is demonstrated using the new X-ray timing results presented here together with a compilation of the previously detected timescales from the literature.



2015 ◽  
Vol 808 (2) ◽  
pp. 163 ◽  
Author(s):  
Hai-Wu Pan ◽  
Weimin Yuan ◽  
Xin-Lin Zhou ◽  
Xiao-Bo Dong ◽  
Bifang Liu


Sign in / Sign up

Export Citation Format

Share Document