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The acceleration of cosmic rays in shock fronts – I

A. R. Bell
- 01 Feb 1978 - 
- Vol. 182, Iss: 2, pp 147-156
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1978-02-01 and is currently open access. It has received 2613 citations till now. The article focuses on the topics: Shock waves in astrophysics & Fermi acceleration.

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Deep morphological and spectral study of the SNR RCW 86 with Fermi-LAT

Marco Ajello, +139 more
TL;DR: In this paper, a broadband modeling of the nonthermal emission of RCW 86 was performed to constrain parameters of the nearby medium and bring new hints about the origin of the γ-ray emission.
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Gyroresonant surfing acceleration.

TL;DR: A new acceleration or energization mechanism of charged particles in space and astrophysical plasmas, in the presence of an electrostatic potential gradient and a circularly polarized electromagnetic monochromatic wave, where particles are accelerated efficiently by keeping cyclotron resonance with the wave due to the electrostatic dragging force.
Journal ArticleDOI

CHAMP Cosmic Rays

TL;DR: In this paper, the authors studied the interactions of cosmological relics, including thermalization with the interstellar medium, diffusion through inhomogeneous magnetic fields and Fermi acceleration by supernova shock waves.
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A Magnetohydrodynamic Model of the M87 Jet I: Superluminal Knot Ejections from HST-1 as Trails of Quad Relativistic MHD Shocks

TL;DR: In this paper, a quad relativistic magnetohydrodynamic shock fronts (forward/reverse fast and slow modes) in a narrow jet with a helically twisted magnetic structure are proposed.
Journal ArticleDOI

Acceleration of cosmic rays by young core-collapse supernova remnants

TL;DR: In this paper, the authors used high-resolution numerical simulations for the hydrodynamical evolution of the supernova remnants (SNRs) and obtained the B-field value at all locations, in particular at the reverse shock.
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