activity
20172022
most citedStratified disc wind models for the AGN broad-line region: ultraviolet, optical and X-ray properties

54 citations · 173 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE202234 cited

Optical line spectra of tidal disruption events from reprocessing in optically thick outflows

Edward J. Parkinson, Christian Knigge, James H. Matthews +4

A significant number of tidal disruption events (TDEs) radiate primarily at optical and ultraviolet (UV) wavelengths, with only weak soft X-ray components. One model for this optic…

astro-ph.HE202035 cited

Thermal and radiation driving can produce observable disk winds in hard-state X-ray binaries

Nick Higginbottom, Christian Knigge, Stuart A. Sim +5

X-ray signatures of outflowing gas have been detected in several accreting black-hole binaries, always in the soft state. A key question raised by these observations is whether the…

astro-ph.GA202054 cited

Stratified disc wind models for the AGN broad-line region: ultraviolet, optical and X-ray properties

James H. Matthews, Christian Knigge, Nick Higginbottom +5

The origin, geometry and kinematics of the broad line region (BLR) gas in quasars and active galactic nuclei (AGN) are uncertain. We demonstrate that clumpy biconical disc winds il…

astro-ph.GA201926 cited

Do Reverberation Mapping Analyses Provide an Accurate Picture of the Broad Line Region?

S. W. Mangham, C. Knigge, P. Williams +6

Reverberation mapping (RM) is a powerful approach for determining the nature of the broad-line region (BLR) in active galactic nuclei. However, inferring physical BLR properties fr…

astro-ph.GA201724 cited

The reverberation signatures of rotating disc winds in active galactic nuclei

S. W. Mangham, C. Knigge, J. H. Matthews +3

The broad emission lines (BELs) in active galactic nuclei (AGN) respond to ionizing continuum variations. The time and velocity dependence of their response depends on the structur…