SUPER-II. Spatially resolved ionised gas kinematics and scaling relations in z∼ 2 AGN host galaxies

D Kakkad, V Mainieri, G Vietri, S Carniani… - Astronomy & …, 2020 - aanda.org
Aims. The SINFONI survey for Unveiling the Physics and Effect of Radiative feedback
(SUPER) aims to trace and characterise ionised gas outflows and their impact on star …

The MAGNUM survey: different gas properties in the outflowing and disc components in nearby active galaxies with MUSE

M Mingozzi, G Cresci, G Venturi, A Marconi… - Astronomy & …, 2019 - aanda.org
We investigated the interstellar medium (ISM) properties of the disc and outflowing gas in
the central regions of nine nearby Seyfert galaxies, all characterised by prominent conical or …

High molecular gas content and star formation rates in local galaxies that host quasars, outflows, and jets

ME Jarvis, CM Harrison, V Mainieri… - Monthly Notices of …, 2020 - academic.oup.com
We use a sample of powerful z\,≈\,0.1 type 2 quasars ('obscured'; log LAGN/erg s ^-
1\,\gtrsim\,45), which host kpc-scale ionized outflows and jets, to identify possible signatures …

Discovering AGN-driven winds through their infrared emission–II. Mass outflow rate and energetics

D Baron, H Netzer - Monthly Notices of the Royal Astronomical …, 2019 - academic.oup.com
The global influence of AGN-driven outflows remains uncertain, due to a lack of large
samples with accurately determined outflow properties. In the second paper of this series …

Positive and negative feedback of AGN outflows in NGC 5728

J Shin, JH Woo, A Chung, J Baek, K Cho… - The Astrophysical …, 2019 - iopscience.iop.org
We present a spatially resolved analysis of ionized and molecular gas in a nearby Seyfert 2
galaxy, NGC 5728, using the Very Large Telescope/MUSE and Atacama Large Millimeter …

MAGNUM survey: A MUSE-Chandra resolved view on ionized outflows and photoionization in the Seyfert galaxy NGC1365

G Venturi, E Nardini, A Marconi, S Carniani… - Astronomy & …, 2018 - aanda.org
Context. Ionized outflows, revealed by broad asymmetric wings of the [O III] λ5007 line, are
commonly observed in active galactic nuclei (AGN) but the low intrinsic spatial resolution of …

arepo-rt: radiation hydrodynamics on a moving mesh

R Kannan, M Vogelsberger, F Marinacci… - Monthly Notices of …, 2019 - academic.oup.com
We introduce arepo-rt, a novel radiation hydrodynamic (RHD) solver for the unstructured
moving-mesh code arepo. Our method solves the moment-based radiative transfer …

The EDGE–CALIFA survey: central molecular gas depletion in AGN host galaxies–a smoking gun for quenching?

SL Ellison, T Wong, SF Sánchez… - Monthly Notices of …, 2021 - academic.oup.com
Feedback from an active galactic nucleus (AGN) is often implicated as a mechanism that
leads to the quenching of galactic star formation. However, AGN-driven quenching is …

The EDGE-CALIFA survey: The role of spiral arms and bars in driving central molecular gas concentrations

SY Yu, V Kalinova, D Colombo, AD Bolatto… - Astronomy & …, 2022 - aanda.org
Shocks and torques produced by non-axisymmetric structures such as spiral arms and bars
may transport gas to galaxy central regions. We test this hypothesis by studying the …

Hubble Space Telescope observations of extended [O III] λ 5007 emission in nearby QSO2s: new constraints on AGN host galaxy interaction

TC Fischer, SB Kraemer, HR Schmitt… - The Astrophysical …, 2018 - iopscience.iop.org
Abstract We present a Hubble Space Telescope survey of extended [O iii] λ5007 emission
for a sample of 12 nearby (z< 0.12), luminous Type 2 quasars (QSO2s), which we use to …