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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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Journal ArticleDOI

Radio Properties of Pinwheel Nebulae

TL;DR: In this article, a radio survey of IR-bright Wolf-Rayet stars was conducted to test the hypothesis that colliding winds lie at the heart of all dusty WR systems.
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Enhanced shock acceleration in relativistic jets and cosmic ray origin in active galactic nuclei

TL;DR: In this article, a numerical simulation of the diffusive shock acceleration process when the flow is relativistic was performed and the acceleration rate was found to be ∼13.5 times faster than the previous values used, which were based on an analytical approximation.
Journal ArticleDOI

Fermi I particle acceleration in converging flows mediated by magnetic reconnection

TL;DR: In this paper, the authors explore the possibility of particles to be accelerated in a magnetic reconnection layer by interacting only with the incoming flows, and derive analytical estimates for the particle energy distribution, acceleration rate, and maximum energies achievable in these flows.
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Acceleration of Ultrahigh-Energy Cosmic Rays in Starburst Superwinds

TL;DR: In this paper, the authors argue that if starbursts are sources of UHECRs, then particle acceleration in the large-scale terminal shock of the superwind that flows from the starburst engine represents the best known concept model in the market.
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