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 …
Jets in radio galaxies and quasars: an observational perspective
DJ Saikia - Journal of Astrophysics and Astronomy, 2022 - Springer
This article gives a brief historical introduction and reviews our current understanding of jets
in radio galaxies and quasars from an observational perspective, with an emphasis on …
in radio galaxies and quasars from an observational perspective, with an emphasis on …
A candidate runaway supermassive black hole identified by shocks and star formation in its wake
P van Dokkum, I Pasha, ML Buzzo… - The Astrophysical …, 2023 - iopscience.iop.org
The interaction of a runaway supermassive black hole (SMBH) with the circumgalactic
medium (CGM) can lead to the formation of a wake of shocked gas and young stars behind …
medium (CGM) can lead to the formation of a wake of shocked gas and young stars behind …
WISDOM project–XIV. SMBH mass in the early-type galaxies NGC 0612, NGC 1574, and NGC 4261 from CO dynamical modelling
We present a CO dynamical estimate of the mass of the supermassive black hole (SMBH) in
three nearby early-type galaxies: NGC 0612, NGC 1574, and NGC 4261. Our analysis is …
three nearby early-type galaxies: NGC 0612, NGC 1574, and NGC 4261. Our analysis is …
Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
We apply a turbulence-regulated model of star formation to calculate the star formation rate
(SFR) of dense star-forming clouds in simulations of jet–interstellar medium (ISM) …
(SFR) of dense star-forming clouds in simulations of jet–interstellar medium (ISM) …
Modelling observable signatures of jet-ISM interaction: thermal emission and gas kinematics
Relativistic jets are believed to have a substantial impact on the gas dynamics and evolution
of the interstellar medium (ISM) of their host galaxies. In this paper, we aim to draw a link …
of the interstellar medium (ISM) of their host galaxies. In this paper, we aim to draw a link …
The large-scale ionization cones in the Galaxy
J Bland-Hawthorn, PR Maloney… - The Astrophysical …, 2019 - iopscience.iop.org
There is compelling evidence for a highly energetic Seyfert explosion (10 56–57 erg) that
occurred in the Galactic center a few million years ago. The clearest indications are the X …
occurred in the Galactic center a few million years ago. The clearest indications are the X …
The AGN fuelling/feedback cycle in nearby radio galaxies–IV. Molecular gas conditions and jet–ISM interaction in NGC 3100
This is the fourth paper of a series investigating the AGN fuelling/feedback processes in a
sample of 11 nearby low-excitation radio galaxies (LERGs). In this paper, we present follow …
sample of 11 nearby low-excitation radio galaxies (LERGs). In this paper, we present follow …
Morphological transition of the compact radio lobe in 3C 84 via the strong jet–cloud collision
M Kino, K Niinuma, N Kawakatu, H Nagai… - The Astrophysical …, 2021 - iopscience.iop.org
We report multiepoch very long baseline interferometric observations of the compact radio
lobe in the radio galaxy 3C 84 (NGC 1275) during 2016–2020. The image sequence of 3C …
lobe in the radio galaxy 3C 84 (NGC 1275) during 2016–2020. The image sequence of 3C …
Jet-driven AGN feedback on molecular gas and low star-formation efficiency in a massive local spiral galaxy with a bright X-ray halo
It has long been suspected that powerful radio sources may lower the efficiency with which
stars form from the molecular gas in their host galaxy, however so far, alternative …
stars form from the molecular gas in their host galaxy, however so far, alternative …