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Cited article:

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A Hydro-based MCMC Analysis of SNR 0509−67.5: Revealing the Explosion Properties from Fluid Discontinuities Alone

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The cosmic ray-driven streaming instability in astrophysical and space plasmas

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Multi-scale simulations of particle acceleration in astrophysical systems

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Interplay between physics and geometry in Balmer filaments: the case of SN 1006

R Bandiera, G Morlino, S Knežević and J C Raymond
Monthly Notices of the Royal Astronomical Society 483 (2) 1537 (2019)
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Balmer-dominated Shocks Exclude Hot Progenitors for Many Type Ia Supernovae

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Multiple Messengers and Challenges in Astroparticle Physics

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Constraints on Cosmic-ray Acceleration Efficiency in Balmer Shocks of Two Young Type Ia Supernova Remnants in the Large Magellanic Cloud

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Three-dimensional Features of the Outer Heliosphere Due to Coupling between the Interstellar and Heliospheric Magnetic Field. V. The Bow Wave, Heliospheric Boundary Layer, Instabilities, and Magnetic Reconnection

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The Highly Collimated Radio Jet of HH 80–81: Structure and Nonthermal Emission

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Ion–Ion Equilibration and Particle Distributions in a 3000 km s−1 Shock in SN 1006

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SECOND EPOCH HUBBLE SPACE TELESCOPE OBSERVATIONS OF KEPLER’S SUPERNOVA REMNANT: THE PROPER MOTIONS OF BALMER FILAMENTS*

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DETECTION OF BROAD Hα EMISSION LINES IN THE LATE-TIME SPECTRA OF A HYDROGEN-POOR SUPERLUMINOUS SUPERNOVA

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A DIRECT MEASUREMENT OF THE FORWARD SHOCK SPEED IN SUPERNOVA REMNANT 0509–67.5: CONSTRAINTS ON THE AGE, AMBIENT DENSITY, SHOCK COMPRESSION FACTOR, AND ELECTRON–ION TEMPERATURE EQUILIBRATION

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