Ordered magnetic fields around the 3C 84 central black hole
Context. 3C 84 is a nearby radio source with a complex total intensity structure, showing
linear polarisation and spectral patterns. A detailed investigation of the central engine region …
linear polarisation and spectral patterns. A detailed investigation of the central engine region …
Enabling transformational ngEHT science via the inclusion of 86 GHz capabilities
We present a case for significantly enhancing the utility and efficiency of the ngEHT by
incorporating an additional 86 GHz observing band. In contrast to 230 or 345 GHz, weather …
incorporating an additional 86 GHz observing band. In contrast to 230 or 345 GHz, weather …
A multi-band study and exploration of the radio wave–γ-ray connection in 3C 84
Total intensity variability light curves offer a unique insight into the ongoing debate about the
launching mechanism of jets. For this work, we utilised the availability of radio and γ-ray light …
launching mechanism of jets. For this work, we utilised the availability of radio and γ-ray light …
Observational evidence to support a dense ambient medium sha** the jet in 3C 84
J Park, M Kino, H Nagai, M Nakamura, K Asada… - Astronomy & …, 2024 - aanda.org
Highly collimated relativistic jets are a defining feature of certain active galactic nuclei
(AGN), yet their formation mechanism remains elusive. Previous observations and …
(AGN), yet their formation mechanism remains elusive. Previous observations and …
[HTML][HTML] Ray-tracing in relativistic jet simulations: A polarimetric study of magnetic field morphology and electron scaling relations
JA Kramer, NR MacDonald - Astronomy & Astrophysics, 2021 - aanda.org
Context. The jets emanating from the centers of active galactic nuclei are among the most
energetic objects in the Universe. Investigating how the morphology of the jet's synchrotron …
energetic objects in the Universe. Investigating how the morphology of the jet's synchrotron …
A persistent double nuclear structure in 3C 84
ABSTRACT 3C 84 (NGC 1275) is the radio source at the centre of the Perseus cluster and
exhibits a bright radio jet. We observed the source with the Global Millimeter VLBI Array …
exhibits a bright radio jet. We observed the source with the Global Millimeter VLBI Array …
Jet kinematics in the transversely stratified jet of 3C 84-A two-decade overview
3C 84 (NGC 1275) is one of the brightest radio sources in the millimetre radio bands, which
led to a plethora of very-long-baseline interferometry (VLBI) observations at numerous …
led to a plethora of very-long-baseline interferometry (VLBI) observations at numerous …
[HTML][HTML] 3D hybrid fluid-particle jet simulations and the importance of synchrotron radiative losses
Context. Relativistic jets in active galactic nuclei are known for their exceptional energy
output, and imaging the synthetic synchrotron emission of numerical jet simulations is …
output, and imaging the synthetic synchrotron emission of numerical jet simulations is …
First very long baseline interferometry detection of Fornax A
Radio galaxies harbouring jetted active galactic nuclei are a frequent target of very long
baseline interferometry (VLBI) because they play an essential role in our exploration of how …
baseline interferometry (VLBI) because they play an essential role in our exploration of how …
RadioAstron discovery of a mini-cocoon around the restarted parsec-scale jet in 3C 84
We present RadioAstron space-based very long baseline interferometry (VLBI) observations
of the nearby radio galaxy 3C 84 (NGC 1275) at the centre of the Perseus cluster. The …
of the nearby radio galaxy 3C 84 (NGC 1275) at the centre of the Perseus cluster. The …