activity
20172026
most citedThe dust-gas AGN torus as constrained from X-ray and mid-infrared observations

39 citations · 65 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Breaking the Blend: A multi-tracer kinematic decomposition method for IFS data applied to disentangling the AGN outflow and circumnuclear ring in NGC 5728 with JWST

Oscar Veenema, Niranjan Thatte, Dimitra Rigopoulou +26

Integral field spectroscopy (IFS) of the central kiloparsecs of active galactic nuclei (AGN) reveals a mixture of spatially coincident emission from star-formation and AGN feedback…

astro-ph.GA2026

Kinematic detection of dusty outflows from active galactic nuclei: Polycyclic aromatic hydrocarbon kinematics of type 2 quasars with JWST/MIRI spectroscopy

Fergus R. Donnan, Cristina Ramos Almeida, Omaira González Martín +5

Active galactic nuclei (AGN) are thought to have dusty outflows, but unlike in the gas phase, it is challenging to measure the kinematics of dust. We present the detection and anal…

astro-ph.GA2025★ 5 cited

Impact of AGN and nuclear star formation on the ISM turbulence of galaxies: Insights from JWST/MIRI spectroscopy

Rogemar A. Riffel, Luis Colina, José Henrique Costa-Souza +31

Active galactic nuclei (AGN), star formation (SF), and galaxy interactions can drive turbulence in the gas of the ISM, which in turn plays a role in the SF within galaxies. The imp…

astro-ph.GA2021★ 39 cited

The dust-gas AGN torus as constrained from X-ray and mid-infrared observations

Donaji Esparza Arredondo, Omaira González Martín, Deborah Dultzin +5

In the last decades, several multiwavelength studies have been dedicated to exploring the properties of the obscuring material in active galactic nuclei (AGN). Various models have…

astro-ph.GA2017★ 21 cited

Star formation in AGNs at the hundred parsec scale using MIR high resolution images

Daniel Ruschel-Dutra, José Miguel Rodríguez Espinosa, Omaira González Martín +2

It has been well established in the past decades that the central black hole masses of galaxies correlate with dynamical properties of their harbouring bulges. This notion begs the…