The acceleration of cosmic rays in shock fronts – I
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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.read more
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A Thousand Days After the Merger: Continued X-Ray Emission From gw170817
E. Troja,E. Troja,H. van Eerten,Bing Zhang,Geoffrey Ryan,Luigi Piro,Roberto Ricci,B. O'Connor,M. H. Wieringa,S. B. Cenko,S. B. Cenko,T. Sakamoto +11 more
TL;DR: In this article, the authors derived an unabsorbed X-ray flux of approximately 1.4E-15 erg/cm^2/s, higher than earlier predictions, yet still consistent with a simple structured jet model.
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Statistical analysis of supernova remnants in the Large Magellanic Cloud
Luke M Bozzetto,Miroslav Filipovic,Branislav Vukotić,Marko Pavlović,Dejan Urošević,Dejan Urošević,Patrick J. Kavanagh,Bojan Arbutina,P. Maggi,Manami Sasaki,Frank Haberl,Evan J Crawford,Quentin Roper,Kevin Grieve,Sean D Points +14 more
TL;DR: The most complete sample of supernova remnants (SNRs) in any galaxy -the Large Magellanic Cloud (LMC) SNR sample was constructed in this article, where the authors studied their various properties such as spectral index, size and surface-brightness.
Journal ArticleDOI
Numerical study of Cosmic Ray Diffusion in MHD turbulence
TL;DR: In this article, the authors studied the diffusion of cosmic ray (CR) in turbulent magnetic fields using test particle simulations and found qualitative correspondence between them in various aspects of CR diffusion.
Journal ArticleDOI
Cosmic‐Ray History and Its Implications for Galactic Magnetic Fields
TL;DR: In this article, the role of magnetic field strength in cosmic-ray acceleration and confinement has been investigated and it has been shown that magnetic fields several orders of magnitude weaker than present galactic fields can accelerate and retain a population of relativistic cosmic rays, provided that the fields are coherent over length scales greater than a cosmic ray gyroradius.
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Radio emission models of colliding-wind binary systems. Inclusion of IC cooling
Julian M. Pittard,Sean M. Dougherty,Robert Coker,Evan O'Connor,Evan O'Connor,N. J. Bolingbroke,N. J. Bolingbroke +6 more
TL;DR: In this paper, the authors extended these models by considering the temporal and spatial evolution of the energy distribution of relativistic electrons as they advect downstream from their shock acceleration site.