most citedMid-infrared variability of changing-look AGN

148 citations · 347 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2017148 cited

Mid-infrared variability of changing-look AGN

Zhenfeng Sheng, Tinggui Wang, Ning Jiang +4

It is known that some active galactic nuclei (AGNs) transited from type 1 to type 2 or vice versa. There are two explanations for the so-called changing look AGNs: one is the drama…

astro-ph.GA201735 cited

Carbon and Nitrogen Abundance Ratio In the Broad Line Region of Tidal Disruption Events

Chenwei Yang, Tinggui Wang, Gary J. Ferland +4

The rest-frame UV spectra of three recent tidal disruption events (TDEs), ASASSN-14li, PTF15af and iPTF16fnl display strong nitrogen emission lines but weak or undetectable carbon…

astro-ph.GA201754 cited

Mid-infrared flare of TDE candidate PS16dtm: dust echo and implications for the spectral evolution

Ning Jiang, Tinggui Wang, Lin Yan +6

PS16dtm was classified as a candidate tidal disruption event (TDE) in a dwarf Seyfert 1 galaxy with low-mass black hole () and has presented various intriguing phot…

astro-ph.HE201711 cited

Numerical Study on Outflows in Seyfert Galaxies I: Narrow Line Region Outflows in NGC 4151

Guobin Mou, Tinggui Wang, Chenwei Yang

The origin of narrow line region (NLR) outflows remains unknown. In this paper, we explore the scenario in which these outflows are circumnuclear clouds driven by energetic accreti…

astro-ph.GA201756 cited

Variation of ionizing continuum: the main driver of Broad Absorption Line Variability

Zhicheng He, Tinggui Wang, Hongyan Zhou +5

We present a statistical analysis of the variability of broad absorption lines (BALs) in quasars using the large multi-epoch spectroscopic dataset of the Sloan Digital Sky Survey D…

astro-ph.GA201543 cited

A Comprehensive Study of Broad Absorption Line Quasars: I. Prevalence of HeI* Absorption Line Multiplets in Low-Ionization Objects

Wen-Juan Liu, Hongyan Zhou, Tuo Ji +13

Neutral Helium multiplets, HeI*3189,3889,10830 are very useful diagnostics to the geometry and physical conditions of the absorbing gas in quasars. So far only a handful of HeI* de…