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Cited article:

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NON-THERMAL X-RAY EMISSION FROM THE NORTHWESTERN RIM OF THE GALACTIC SUPERNOVA REMNANT G266.2–1.2 (RX J0852.0-4622)

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Confinement and anisotropy of ultrahigh-energy cosmic rays in isotropic plasma wave turbulence

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Dynamics of Mesoscale Magnetic Field in Diffusive Shock Acceleration

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A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7–3946 with HESS

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Cosmic‐Ray Propagation Properties for an Origin in Supernova Remnants

I. Busching, A. Kopp, M. Pohl, et al.
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A Detailed Study of Molecular Clouds toward the TeV Gamma‐Ray Supernova Remnant G347.3−0.5

Y. Moriguchi, K. Tamura, Y. Tawara, et al.
The Astrophysical Journal 631 (2) 947 (2005)
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Multiwavelength spectral models for SNR G347.3-0.5 from non-linear shock acceleration

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On the Gamma-Ray Spectra Radiated by Protons Accelerated in Supernova Remnant Shocks near Molecular Clouds: The case of Supernova Remnant RX J1713.7-3946

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The Most Likely Sources of High‐Energy Cosmic‐Ray Electrons in Supernova Remnants

T. Kobayashi, Y. Komori, K. Yoshida and J. Nishimura
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A High‐Resolution Study of Nonthermal Radio and X‐Ray Emission from Supernova Remnant G347.3−0.5

J. S. Lazendic, P. O. Slane, B. M. Gaensler, et al.
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The Origin of Nonthermal X‐Ray Filaments and TeV Emission in Young Supernova Remnants

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XMM-Newtonobservations of the supernova remnant RX J1713.7–3946 and its central source

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XMM-Newton Observation of SNR RX J1713.7–3946

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Hydrodynamic simulation of supernova remnants including efficient particle acceleration

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RXTE,ROSAT, andASCAObservations of G347.3−0.5 (RX J1713.7−3946): Probing Cosmic‐Ray Acceleration by a Galactic Shell‐Type Supernova Remnant

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Flat Spectrum X-Ray Emission from the Direction of a Molecular Cloud Associated with SNR RX J1713.7–3946

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Possible High-Energy Neutrinos from the Cosmic Accelerator RX J1713.7−3946

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