Results 161 to 170 of about 1,046 (208)

Heavy-element production in a compact object merger observed by JWST. [PDF]

open access: yesNature
Levan AJ   +84 more
europepmc   +1 more source

HARD X-RAY EMISSION DURING FLARES AND PHOTOSPHERIC FIELD CHANGES. [PDF]

open access: yesAstrophys J, 2015
Burtseva O   +3 more
europepmc   +1 more source

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies. [PDF]

open access: yesOpen Res Eur
Liu D   +27 more
europepmc   +1 more source

Magnetohydrodynamic Simulations of the Geodynamo

open access: yes, 2003
Harder, Helmut   +2 more
openaire   +1 more source

Black hole jets on the scale of the Cosmic Web

open access: yes
Oei MS   +12 more
europepmc   +1 more source

A test suite for magnetohydrodynamical simulations

open access: yesAstrophysical Journal, 1992
A collection is presented of MHD problems that will provide researchers who have interests in modeling MHD phenomena with a battery of tests (a 'test suite') for calibrating their numerical algorithms. Use of these tests will provide a common reference for comparison of different numerical MHD algorithms. The test suite includes both 1D and 2D problems.
John F Hawley   +2 more
exaly   +4 more sources

Evolution of cosmic ray electron spectra in magnetohydrodynamical simulations

open access: yesMonthly Notices of the Royal Astronomical Society, 2019
Cosmic ray (CR) electrons reveal key insights into the non-thermal physics of the interstellar medium (ISM), galaxies, galaxy clusters, and active galactic nuclei by means of their inverse Compton (IC) γ -ray emission and synchrotron emission in magnetic
Georg Winner   +2 more
exaly   +2 more sources

Three-dimensional Magnetohydrodynamical Simulations of the Morphology of Head–Tail Radio Galaxies Based on the Magnetic Tower Jet Model

open access: yesAstrophysical Journal, 2017
The distinctive morphology of head–tail radio galaxies reveals strong interactions between the radio jets and their intra-cluster environment, the general consensus on the morphology origin of head–tail sources is that radio jets are bent by violent ...
Zhaoming Gan, Hui Li, Shengtai Li
exaly   +2 more sources

Relativistic magnetohydrodynamical simulations of the resonant corrugation of a fast shock front

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
The generation of turbulence at magnetized shocks and its subsequent interaction with the latter is a key question of plasma- and high-energy astrophysics.
Camilia Demidem   +2 more
exaly   +2 more sources

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