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Magnetic field amplification in Tycho and other shell-type supernova remnants
It is shown that amplification of the magnetic field in supernova remnants (SNRs) occurs in all six objects where morphological measurements are presently available in the hard X-ray continuum at
Detection of sub-TeV gamma-rays from the Galactic Center direction by CANGAROO-II
K. Tsuchiya, R. Enomoto, L. T. Ksenofontov, M. Mori, T. Naito, A. Asahara, G. V. Bicknell, R. W. Clay, Y. Doi, P. G. Edwards, S. Gunji, S. Hara, T. Hara, T. Hattori, Sei. Hayashi, C. Itoh, S. Kabuki,
Confirmation of strong magnetic field amplification and nuclear cosmic ray acceleration in SN 1006
It is shown that the nonlinear kinetic model of cosmic ray (CR) acceleration in supernova remnants (SNRs) fits the shell-type nonthermal X-ray morphology, obtained in Chandra observations, in a
Cosmic ray acceleration parameters from multi-wavelength observations. The case of SN 1006
Aims. The properties of the Galactic supernova remnant (SNR) SN 1006 are theoretically reanalysed. Methods. Nonlinear kinetic theory is used to determine the accelerat ion efficiency of cosmic rays
The Large High Altitude Air Shower Observatory (LHAASO) Science White Paper
The Large High Altitude Air Shower Observatory (LHAASO) project is a new generation multi-component instrument, to be built at 4410 meters of altitude in the Sichuan province of China, with the aim
The Nature of Gamma-Ray Emission of Tycho's Supernova Remnant
The nature of the recently detected high-energy and very high-energy ?-ray emission of Tycho's supernova remnant (SNR) is studied. A nonlinear kinetic theory of cosmic-ray (CR) acceleration in SNRs
The high energy gamma-ray emission expected from Tycho's supernova remnant
A nonlinear kinetic model of cosmic ray (CR) acceleration in supernova remnants (SNRs) is used to describe the properties of Tycho's SNR. Observations of the expansion characteristics and of the
Dependence of the gamma-ray emission from SN 1006 on the astronomical parameters
We use nonlinear kinetic theory to study the remnant dynamics and the particle acceleration as well as the properties of the nonthermal emission from the supernova remnant SN 1006. The known range of
Detection of Gamma Rays around 1 TeV from RX J0852.0–4622 by CANGAROO-II
We have detected gamma-ray emission at the 6 σ level at energies greater than 500 GeV from the supernova remnant RX J0852.0-4622 (G266.2-1.2) using the CANGAROO-II imaging atmospheric Cerenkov
Emission of SN 1006 produced by accelerated cosmic rays
The nonlinear kinetic model of cosmic ray (CR) acceleration in supernova remnants (SNRs) is used to describe the properties of the remnant of SN 1006. It is shown, that the theory fits the existing
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