Compact steep-spectrum and peaked-spectrum radio sources
CP O'Dea, DJ Saikia - The Astronomy and Astrophysics Review, 2021 - Springer
Compact steep-spectrum (CSS) and peaked-spectrum (PS) radio sources are compact,
powerful radio sources. The multi-frequency observational properties and current theories …
powerful radio sources. The multi-frequency observational properties and current theories …
What drives the growth of black holes?
DM Alexander, RC Hickox - New Astronomy Reviews, 2012 - Elsevier
Massive black holes (BHs) are at once exotic and yet ubiquitous, residing at the centers of
massive galaxies in the local Universe. Recent years have seen remarkable advances in …
massive galaxies in the local Universe. Recent years have seen remarkable advances in …
Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population
CM Harrison, DM Alexander… - Monthly Notices of …, 2014 - academic.oup.com
We present integral field unit observations covering the [o iii] λλ4959, 5007 and Hβ emission
lines of 16 z< 0.2 type 2 active galactic nuclei (AGN). Our targets are selected from a well …
lines of 16 z< 0.2 type 2 active galactic nuclei (AGN). Our targets are selected from a well …
Galaxy pairs in the Sloan Digital Sky Survey–IV. Interactions trigger active galactic nuclei
Galaxy–galaxy interactions are predicted to cause gas inflows leading to enhanced nuclear
star formation. This prediction is borne out observationally, and is also supported by the gas …
star formation. This prediction is borne out observationally, and is also supported by the gas …
The diverse cold molecular gas contents, morphologies, and kinematics of type-2 quasars as seen by ALMA
CR Almeida, M Bischetti, S García-Burillo… - Astronomy & …, 2022 - aanda.org
We present CO (2− 1) and adjacent continuum observations of seven nearby radio-quiet
type-2 quasars (QSO2s) obtained with ALMA at∼ 0.2 ″resolution (370 pc at z∼ 0.1). These …
type-2 quasars (QSO2s) obtained with ALMA at∼ 0.2 ″resolution (370 pc at z∼ 0.1). These …
Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured
Mergers of galaxies are thought to cause significant gas inflows to the inner parsecs, which
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …
A definitive merger-AGN connection at z ∼ 0 with CFIS: mergers have an excess of AGN and AGN hosts are more frequently disturbed
The question of whether galaxy mergers are linked to the triggering of active galactic nuclei
(AGN) continues to be a topic of considerable debate. The issue can be broken down into …
(AGN) continues to be a topic of considerable debate. The issue can be broken down into …
Galaxy interactions are the dominant trigger for local type 2 quasars
JCS Pierce, C Tadhunter… - Monthly Notices of …, 2023 - academic.oup.com
The triggering mechanism for the most luminous, quasar-like active galactic nuclei (AGN)
remains a source of debate, with some studies favouring triggering via galaxy mergers, but …
remains a source of debate, with some studies favouring triggering via galaxy mergers, but …
Galaxy pairs in the Sloan Digital Sky Survey–VIII. The observational properties of post-merger galaxies
In order to investigate the effects of galaxy mergers throughout the interaction sequence, we
present a study of 10 800 galaxies in close pairs and a smaller sample of 97 post-mergers …
present a study of 10 800 galaxies in close pairs and a smaller sample of 97 post-mergers …
Interacting galaxies in the IllustrisTNG simulations− IV: enhanced supermassive black hole accretion rates in post-merger galaxies
S Byrne-Mamahit, MH Hani, SL Ellison… - Monthly Notices of …, 2023 - academic.oup.com
We present an analysis of the instantaneous supermassive black hole (SMBH) accretion
rates in a collection of 1563 post-merger galaxies drawn from the IllustrisTNG simulation …
rates in a collection of 1563 post-merger galaxies drawn from the IllustrisTNG simulation …