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Cited article:

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LOCALIZED SiO EMISSION TRIGGERED BY THE PASSAGE OF THE W51C SUPERNOVA REMNANT SHOCK

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THREE-DIMENSIONAL SIMULATIONS OF THE NON-THERMAL BROADBAND EMISSION FROM YOUNG SUPERNOVA REMNANTS INCLUDING EFFICIENT PARTICLE ACCELERATION

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DETAILED INVESTIGATION OF THE GAMMA-RAY EMISSION IN THE VICINITY OF SNR W28 WITHFERMI-LAT

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Acceleration of cosmic rays and gamma-ray emission from supernova remnants in the Galaxy

P. Cristofari, S. Gabici, S. Casanova, R. Terrier and E. Parizot
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Exploring the  -ray emissivity of young supernova remnants - I. Hadronic emission

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Gamma-ray signatures of cosmic ray acceleration, propagation, and confinement in the era of CTA

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Propagation of galactic cosmic rays in the presence of self-generated turbulence

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Recombining Plasma and Hard X-Ray Filament in the Mixed-Morphology Supernova Remnant W 44

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NONTHERMAL EMISSION OF SUPERNOVA REMNANT SN 1006 REVISITED: THEORETICAL MODEL AND THE H.E.S.S. RESULTS

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Analysis of Lateral Distribution of Atmospheric Cherenkov Light at High Mountain Altitude Towards Event Reconstruction

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Alfvén wave amplification and self-containment of cosmic rays escaping from a supernova remnant

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Monthly Notices of the Royal Astronomical Society 415 (4) 3434 (2011)
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Analysis of the possibility of describing the phase and amplitude of cosmic ray proton anisotropy and electron spectra in the 1-TeV range within one set of nearby sources

L. G. Sveshnikova, V. S. Ptuskin and O. N. Strelnikova
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