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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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Probing the local environment of the supernova remnant HESS J1731-347 with CO and CS observations

TL;DR: In this paper, the authors discuss the importance of Braiding and Braiding's Braiding Braiding, G.N. Maxted, M. Burton, C. Rowell, H. Sano, F. Voisin, M C. Capasso, G Puhlhofer and Y. Fukui
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Modelling the cosmic ray electron propagation in M 51

TL;DR: In this article, an isotropic diffusion coefficient with a value of 6.6 ± 0.2 × 1028 cm2 s-1 is found to fit best and is similar to what is seen in the Milky Way.
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XMM-Newton and INTEGRAL analysis of the Ophiuchus cluster of galaxies

TL;DR: In this article, the authors investigated the non-thermal hard X-ray emission in the Ophiuchus cluster of galaxies and investigated the physical properties of the nonthermal component and its interaction with the cosmic microwave background.
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Gamma rays as probes of cosmic-ray propagation and interactions in galaxies.

TL;DR: Gamma-ray observations have been pushing forward our understanding of the life cycle of cosmic rays in galaxies and, combined with advances in related domains, they have been challenging standard assumptions in the field and have spurred new developments in modelling approaches and data analysis methods as discussed by the authors.
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