Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
The microphysics of collisionless shock waves
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 …
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 …
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 …
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 …
(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
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 …
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
Using three-dimensional magnetohydrodynamic simulations, we investigate general
properties of a blast wave shock interacting with interstellar clouds. The pre-shock cloudy …
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 …
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 …
(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
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 …
(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
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 …
vicinity of a shock front leads to predict the appearance of a non-Alfvénic fast-growing mode …