Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical …
M Ruszkowski, C Pfrommer - The Astronomy and Astrophysics Review, 2023 - Springer
Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …
Radio galaxies and feedback from AGN jets
MJ Hardcastle, JH Croston - New Astronomy Reviews, 2020 - Elsevier
We review current understanding of the population of radio galaxies and radio-loud quasars
from an observational perspective, focusing on their large-scale structures and dynamics …
from an observational perspective, focusing on their large-scale structures and dynamics …
First M87 event horizon telescope results. VIII. Magnetic field structure near the event horizon
Abstract Event Horizon Telescope (EHT) observations at 230GHz have now imaged
polarized emission around the supermassive black hole in M87 on event-horizon scales …
polarized emission around the supermassive black hole in M87 on event-horizon scales …
[HTML][HTML] First M87 event horizon telescope results. IV. Imaging the central supermassive black hole
First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
- IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
- IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
First M87 event horizon telescope results. V. Physical origin of the asymmetric ring
Abstract The Event Horizon Telescope (EHT) has mapped the central compact radio source
of the elliptical galaxy M87 at 1.3 mm with unprecedented angular resolution. Here we …
of the elliptical galaxy M87 at 1.3 mm with unprecedented angular resolution. Here we …
First M87 event horizon telescope results. I. The shadow of the supermassive black hole
Event Horizon Telescope Collaboration - arXiv preprint arXiv …, 2019 - arxiv.org
When surrounded by a transparent emission region, black holes are expected to reveal a
dark shadow caused by gravitational light bending and photon capture at the event horizon …
dark shadow caused by gravitational light bending and photon capture at the event horizon …
Jets in magnetically arrested hot accretion flows: Geometry, power, and black hole spin-down
We present the results of nine simulations of radiatively inefficient magnetically arrested
discs (MADs) across different values of the black hole spin parameter a*:− 0.9,− 0.7,− 0.5 …
discs (MADs) across different values of the black hole spin parameter a*:− 0.9,− 0.7,− 0.5 …
Polarimetric properties of Event Horizon Telescope targets from ALMA
C Goddi, I Martí-Vidal, H Messias… - The Astrophysical …, 2021 - iopscience.iop.org
We present the results from a full polarization study carried out with the Atacama Large
Millimeter/submillimeter Array (ALMA) during the first Very Long Baseline Interferometry …
Millimeter/submillimeter Array (ALMA) during the first Very Long Baseline Interferometry …
LOFAR: The low-frequency array
MP van Haarlem, MW Wise, AW Gunst, G Heald… - Astronomy & …, 2013 - aanda.org
LOFAR, the LOw-Frequency ARray, is a new-generation radio interferometer constructed in
the north of the Netherlands and across europe. Utilizing a novel phased-array design …
the north of the Netherlands and across europe. Utilizing a novel phased-array design …
General relativistic magnetohydrodynamical simulations of the jet in M 87
M Mościbrodzka, H Falcke, H Shiokawa - Astronomy & Astrophysics, 2016 - aanda.org
Context. The connection between black hole, accretion disk, and radio jet can be
constrained best by fitting models to observations of nearby low-luminosity galactic nuclei, in …
constrained best by fitting models to observations of nearby low-luminosity galactic nuclei, in …