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Theory of cosmic ray and γ-ray production in the supernova remnant RX J0852.0-4622

E. G. Berezhko, G. Pühlhofer and H. J. Völk
Astronomy & Astrophysics 505 (2) 641 (2009)
DOI: 10.1051/0004-6361/200809473
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Simulating TeV gamma-ray morphologies of shell-type supernova remnants

Matteo Pais and Christoph Pfrommer
Monthly Notices of the Royal Astronomical Society 498 (4) 5557 (2020)
DOI: 10.1093/mnras/staa2827
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The Origin of Nonthermal X‐Ray Filaments and TeV Emission in Young Supernova Remnants

M. Lyutikov and M. Pohl
The Astrophysical Journal 609 (2) 785 (2004)
DOI: 10.1086/421290
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Astrophysical origins of ultrahigh energy cosmic rays

Diego F Torres and Luis A Anchordoqui
Reports on Progress in Physics 67 (9) 1663 (2004)
DOI: 10.1088/0034-4885/67/9/R03
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The Contribution of Different Supernova Populations to the Galactic Gamma‐Ray Background

E. G. Berezhko and H. J. Volk
The Astrophysical Journal 611 (1) 12 (2004)
DOI: 10.1086/421937
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Imprint of Intergalactic Shocks on the Radio Sky

Uri Keshet, Eli Waxman and Abraham Loeb
The Astrophysical Journal 617 (1) 281 (2004)
DOI: 10.1086/424837
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Radio, X-ray, and γ-ray emission models of the colliding-wind binary WR 140

J. M. Pittard and S. M. Dougherty
Monthly Notices of the Royal Astronomical Society 372 (2) 801 (2006)
DOI: 10.1111/j.1365-2966.2006.10888.x
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Gamma-ray emission expected from Kepler’s SNR

E. G. Berezhko, L. T. Ksenofontov and H. J. Völk
Astrophysics and Space Science 309 (1-4) 385 (2007)
DOI: 10.1007/s10509-007-9401-3
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The Multi-Messenger Approach to High-Energy Gamma-Ray Sources

E. G. Berezhko, L. T. Ksenofontov and H. J. Völk
The Multi-Messenger Approach to High-Energy Gamma-Ray Sources 385 (2007)
DOI: 10.1007/978-1-4020-6118-9_59
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Diffuse radio emission from clusters in the MareNostrum Universe simulation

M. Hoeft, M. Brüggen, G. Yepes, S. Gottlöber and A. Schwope
Monthly Notices of the Royal Astronomical Society 391 (4) 1511 (2008)
DOI: 10.1111/j.1365-2966.2008.13955.x
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The Multi-Messenger Approach to High-Energy Gamma-Ray Sources

H. J. Völk, E. G. Berezhko and L. T. Ksenofontov
The Multi-Messenger Approach to High-Energy Gamma-Ray Sources 389 (2007)
DOI: 10.1007/978-1-4020-6118-9_60
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Postshock turbulence and diffusive shock acceleration in young supernova remnants

A. Marcowith and F. Casse
Astronomy and Astrophysics 515 A90 (2010)
DOI: 10.1051/0004-6361/200913022
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Spatial structure of X-ray filaments in SN 1006

G. Morlino, E. Amato, P. Blasi and D. Caprioli
Monthly Notices of the Royal Astronomical Society: Letters 405 (1) L21 (2010)
DOI: 10.1111/j.1745-3933.2010.00851.x
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Reviews in Modern Astronomy

Dieter Horns
Reviews in Modern Astronomy 167 (2008)
DOI: 10.1002/9783527622993.ch8
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Cosmic ray models

M. Kachelrieß and D.V. Semikoz
Progress in Particle and Nuclear Physics 109 103710 (2019)
DOI: 10.1016/j.ppnp.2019.07.002
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THE NONLINEAR SATURATION OF THE NON-RESONANT KINETICALLY DRIVEN STREAMING INSTABILITY

L. Gargaté, R. A. Fonseca, J. Niemiec, et al.
The Astrophysical Journal 711 (2) L127 (2010)
DOI: 10.1088/2041-8205/711/2/L127
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Light and Heavy Cosmic-Ray Mass Group Energy Spectra as Measured by the MAKET-ANI Detector

A. Chilingarian, G. Gharagyozyan, G. Hovsepyan, et al.
The Astrophysical Journal 603 (1) L29 (2004)
DOI: 10.1086/383086
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Magnetically Limited X-Ray Filaments in Young Supernova Remnants

M. Pohl, H. Yan and A. Lazarian
The Astrophysical Journal 626 (2) L101 (2005)
DOI: 10.1086/431902
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Magnetic Field Amplification by Shocks in Turbulent Fluids

J. Giacalone and J. R. Jokipii
The Astrophysical Journal 663 (1) L41 (2007)
DOI: 10.1086/519994
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PLASMA INSTABILITIES AS A RESULT OF CHARGE EXCHANGE IN THE DOWNSTREAM REGION OF SUPERNOVA REMNANT SHOCKS

Yutaka Ohira, Toshio Terasawa and Fumio Takahara
The Astrophysical Journal 703 (1) L59 (2009)
DOI: 10.1088/0004-637X/703/1/L59
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Cosmic-ray acceleration and escape from post-adiabatic supernova remnants

R. Brose, M. Pohl, I. Sushch, O. Petruk and T. Kuzyo
Astronomy & Astrophysics 634 A59 (2020)
DOI: 10.1051/0004-6361/201936567
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Magnetic field amplification in Tycho and other shell-type supernova remnants

H. J. Völk, E. G. Berezhko and L. T. Ksenofontov
Astronomy & Astrophysics 433 (1) 229 (2005)
DOI: 10.1051/0004-6361:20042015
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