The microphysics of collisionless shock waves

A Marcowith, A Bret, A Bykov… - Reports on Progress …, 2016 - iopscience.iop.org
Collisionless shocks, that is shocks mediated by electromagnetic processes, are customary
in space physics and in astrophysics. They are to be found in a great variety of objects and …

Observational signatures of particle acceleration in supernova remnants

EA Helder, J Vink, AM Bykov, Y Ohira… - Space Science …, 2012 - Springer
We evaluate the current status of supernova remnants as the sources of Galactic cosmic
rays. We summarize observations of supernova remnants, covering the whole …

Supernova remnants: the X-ray perspective

J Vink - The Astronomy and Astrophysics Review, 2012 - Springer
Supernova remnants are beautiful astronomical objects that are also of high scientific
interest, because they provide insights into supernova explosion mechanisms, and because …

Strong evidence for hadron acceleration in Tycho's supernova remnant

G Morlino, D Caprioli - Astronomy & Astrophysics, 2012 - aanda.org
Context. Very recent gamma-ray observations of G120. 1+ 1.4 (Tycho's) supernova remnant
(SNR) by Fermi-LAT and VERITAS have provided new fundamental pieces of information for …

Observations of the young supernova remnant RX J1713. 7− 3946 with the Fermi Large Area Telescope

AA Abdo, M Ackermann, M Ajello… - The Astrophysical …, 2011 - iopscience.iop.org
We present observations of the young supernova remnant (SNR) RX J1713. 7− 3946 with
the Fermi Large Area Telescope (LAT). We clearly detect a source positionally coincident …

Toward understanding the cosmic-ray acceleration at young supernova remnants interacting with interstellar clouds: possible applications to RX J1713. 7− 3946

T Inoue, R Yamazaki, S Inutsuka… - The Astrophysical …, 2011 - iopscience.iop.org
Using three-dimensional magnetohydrodynamic simulations, we investigate general
properties of a blast wave shock interacting with interstellar clouds. The pre-shock cloudy …

Cosmic-ray acceleration at the forward shock in Tycho's supernova remnant: evidence from Chandra X-ray observations

JS Warren, JP Hughes, C Badenes… - The Astrophysical …, 2005 - iopscience.iop.org
We present evidence for cosmic-ray acceleration at the forward shock in Tycho's supernova
remnant (SNR) from three X-ray observables:(1) the proximity of the contact discontinuity to …

Observational constraints on energetic particle diffusion in young supernovae remnants: amplified magnetic field and maximum energy

E Parizot, A Marcowith, J Ballet, YA Gallant - Astronomy & Astrophysics, 2006 - aanda.org
Constraints on the diffusion and acceleration parameters in five young supernova remnants
(SNRs) are derived from the observed thickness of their X-ray rims, as limited by the …

Magnetic fields in supernova remnants and pulsar-wind nebulae

SP Reynolds, BM Gaensler, F Bocchino - Space science reviews, 2012 - Springer
We review the observations of supernova remnants (SNRs) and pulsar-wind nebulae
(PWNe) that give information on the strength and orientation of magnetic fields. Radio …

A kinetic approach to cosmic-ray-induced streaming instability at supernova shocks

E Amato, P Blasi - Monthly Notices of the Royal Astronomical …, 2009 - academic.oup.com
We show that a purely kinetic approach to the excitation of waves by cosmic rays in the
vicinity of a shock front leads to predict the appearance of a non-Alfvénic fast-growing mode …