[HTML][HTML] Grid-based methods in relativistic hydrodynamics and magnetohydrodynamics
JM Martí, E Müller - Living reviews in computational astrophysics, 2015 - Springer
An overview of grid-based numerical methods used in relativistic hydrodynamics (RHD) and
magnetohydrodynamics (RMHD) is presented. Special emphasis is put on a comprehensive …
magnetohydrodynamics (RMHD) is presented. Special emphasis is put on a comprehensive …
Dissipative processes and their role in the evolution of radio galaxies
M Perucho - Galaxies, 2019 - mdpi.com
Particle acceleration in relativistic jets, to very high levels of energy, occurs at the expense of
the dissipation of magnetic or kinetic energy. Therefore, understanding the processes that …
the dissipation of magnetic or kinetic energy. Therefore, understanding the processes that …
Simulating the dynamics and non-thermal emission of relativistic magnetized jets I. Dynamics
We have performed magnetohydrodynamic (MHD) simulations of relativistic jets from
supermassive blackholes over a few tens of kpc for a range of jet parameters. One of the …
supermassive blackholes over a few tens of kpc for a range of jet parameters. One of the …
Particle acceleration in shearing flows: the self-generation of turbulent spine-sheath structures in relativistic magnetohydrodynamic jet simulations
ABSTRACT X-ray observations of kiloparsec-scale extragalactic jets favour a synchrotron
origin. The short cooling times of the emitting electrons require a distributed acceleration of …
origin. The short cooling times of the emitting electrons require a distributed acceleration of …
Catching the radio flare in CTA 102-III. Core-shift and spectral analysis
Context. The temporal and spatial spectral evolution of the jets of active galactic nuclei
(AGN) can be studied with multi-frequency, multi-epoch very-long-baseline-interferometry …
(AGN) can be studied with multi-frequency, multi-epoch very-long-baseline-interferometry …
Long-term FRII jet evolution: clues from three-dimensional simulations
We present a long-term numerical 3D simulation of a relativistic outflow designed to be
compared with previous results from axisymmetric, 2D simulations, with existing analytical …
compared with previous results from axisymmetric, 2D simulations, with existing analytical …
Instability of supersonic cold streams feeding galaxies–I. Linear Kelvin–Helmholtz instability with body modes
Massive galaxies at high redshift are predicted to be fed from the cosmic web by narrow,
dense streams of cold gas that penetrate through the hot medium encompassed by a stable …
dense streams of cold gas that penetrate through the hot medium encompassed by a stable …
Three-dimensional relativistic magnetohydrodynamic simulations of magnetized spine-sheath relativistic jets
Numerical simulations of weakly and strongly magnetized relativistic jets embedded in a
weakly magnetized and strongly magnetized stationary or weakly relativistic (v= c/2) sheath …
weakly magnetized and strongly magnetized stationary or weakly relativistic (v= c/2) sheath …
Erratic jet wobbling in the BL lacertae object OJ287 revealed by sixteen years of 7 mm VLBA observations
I Agudo, AP Marscher, SG Jorstad… - The Astrophysical …, 2012 - iopscience.iop.org
We present the results from an ultra-high-resolution 7 mm Very Long Baseline Array study of
the relativistic jet in the BL Lacertae object OJ287 from 1995 to 2011 containing 136 total …
the relativistic jet in the BL Lacertae object OJ287 from 1995 to 2011 containing 136 total …
Propagation, cocoon formation, and resultant destabilization of relativistic jets
J Matsumoto, Y Masada - Monthly Notices of the Royal …, 2019 - academic.oup.com
ABSTRACT A cocoon is a by-product of a propagating jet that results from shock heating at
the jet head. Herein, considering simultaneous cocoon formation, we study the stability of …
the jet head. Herein, considering simultaneous cocoon formation, we study the stability of …