328 citations · 3.7k across the 83 of their papers we have counts for
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No Small Scale Radio Jets Here: Multi-Epoch Observations of Radio Continuum Structures in NGC 1068 with the VLBA
Travis C. Fischer, Megan C. Johnson, Nathan J. Secrest +2
We present recent Very Long Baseline Array (VLBA) 5 GHz radio observations of the nearby, luminous Seyfert 2 galaxy NGC 1068 for comparison to similar VLBA observations made on 199…
Investigating the Narrow Line Region Dynamics in Nearby Active Galaxies
Beena Meena, D. Michael Crenshaw, Henrique R. Schmitt +7
We present dynamical models of the narrow line region (NLR) outflows in the nearby Seyfert galaxies Mrk 3, Mrk 78, NGC 1068, and NGC 4151 using observations from the Hubble Space T…
Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. IV. The Effects of Different Density Estimates on the Ionized Gas Masses and Outflow Rates
Mitchell Revalski, D. Michael Crenshaw, Marc Rafelski +9
Active galactic nuclei (AGN) can launch outflows of ionized gas that may influence galaxy evolution, and quantifying their full impact requires spatially resolved measurements of t…
Tracking X-ray Outflows with Optical/IR Footprint Lines
Anna Trindade Falcao, S. B. Kraemer, D. M. Crenshaw +5
We use Cloudy photoionisation models to predict the flux profiles for optical/IR emission lines that trace the footprint of X-ray gas, such as [Fe X] 6375A and [Si X] 1.43m. The…
Hubble Space Telescope [O III] Emission-Line Kinematics in Two Nearby QSO2s: A Case for X-ray Feedback
Anna Trindade Falcão, S. B. Kraemer, T. C. Fischer +15
We present a dynamical study of the narrow-line regions in two nearby QSO2s. We construct dynamical models based on detailed photoionization models of the emission-line gas, includ…
Gauging the effect of Supermassive Black Holes feedback on Quasar host galaxies
B. Dall'Agnol de Oliveira, T. Storchi-Bergmann, S. B. Kraemer +6
In order to gauge the role that active galactic nuclei (AGN) play in the evolution of galaxies via the effect of kinetic feedback in nearby QSO2's (), we observed eig…