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Cited article:

Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton γ-ray morphology of supernova remnants

S. Orlando, O. Petruk, F. Bocchino, M. Miceli

A&A, 526 (2011) A129

Published online: 2011-01-11

DOI: https://doi.org/10.1051/0004-6361/201015505

This article has been cited by the following article(s):

Radio, X-ray and γ-ray surface brightness profiles as powerful diagnostic tools for non-thermal SNR shells

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Monthly Notices of the Royal Astronomical Society 413 (3) 1657 (2011)
DOI: 10.1111/j.1365-2966.2011.18239.x
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A blowout numerical model for the supernova remnant G352.7−0.1

J. C. Toledo-Roy, P. F. Velázquez, A. Esquivel and E. Giacani
Monthly Notices of the Royal Astronomical Society 437 (1) 898 (2014)
DOI: 10.1093/mnras/stt1955
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Radio polarization maps of shell-type SNRs – II. Sedov models with evolution of turbulent magnetic field

O. Petruk, R. Bandiera, V. Beshley, S. Orlando and M. Miceli
Monthly Notices of the Royal Astronomical Society 470 (1) 1156 (2017)
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ROLE OF EJECTA CLUMPING AND BACK-REACTION OF ACCELERATED COSMIC RAYS IN THE EVOLUTION OF TYPE Ia SUPERNOVA REMNANTS

S. Orlando, F. Bocchino, M. Miceli, O. Petruk and M. L. Pumo
The Astrophysical Journal 749 (2) 156 (2012)
DOI: 10.1088/0004-637X/749/2/156
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3D MHD modeling of the expanding remnant of SN 1987A

S. Orlando, M. Miceli, O. Petruk, et al.
Astronomy & Astrophysics 622 A73 (2019)
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Numerically modelling the Cygnus Loop as a remnant evolved in an anisotropic cavity

Jun Fang, Huan Yu and Li Zhang
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Hadronic γ-ray images of Sedov supernova remnants

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Electron and ion acceleration in relativistic shocks with applications to GRB afterglows

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Observational constraints on the modelling of SN 1006

O. Petruk, V. Beshley, F. Bocchino, M. Miceli and S. Orlando
Monthly Notices of the Royal Astronomical Society 413 (3) 1643 (2011)
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THREE-DIMENSIONAL SIMULATIONS OF THE THERMAL X-RAY EMISSION FROM YOUNG SUPERNOVA REMNANTS INCLUDING EFFICIENT PARTICLE ACCELERATION

Gilles Ferrand, Anne Decourchelle and Samar Safi-Harb
The Astrophysical Journal 760 (1) 34 (2012)
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Three-dimensional magnetohydrodynamic studies of the non-thermal X-ray morphologies of SN 1006

Huan Yu, Jun Fang, Peng Fei Zhang and Li Zhang
Astronomy & Astrophysics 579 A35 (2015)
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Constraints on the local interstellar magnetic field from non-thermal emission of SN1006

F. Bocchino, S. Orlando, M. Miceli and O. Petruk
Astronomy & Astrophysics 531 A129 (2011)
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Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray andγ-ray emission

M. Miceli, S. Orlando, V. Pereira, et al.
Astronomy & Astrophysics 593 A26 (2016)
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Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment

O Petruk, T Kuzyo, S Orlando, et al.
Monthly Notices of the Royal Astronomical Society 479 (3) 4253 (2018)
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A method for computing synchrotron and inverse-Compton emission from hydrodynamic simulations of supernova remnants

M. Obergaulinger, J.M. Chimeno, P. Mimica, M.Á. Aloy and A. Iyudin
High Energy Density Physics 17 92 (2015)
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