81 citations · 85 across the 2 of their papers we have counts for
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The radio expansion and brightening of the very young supernova remnant G1.9+0.3
D. A. Green, S. P. Reynolds, K. J. Borkowski +3
Recent radio observations of the small Galactic supernova remnant G1.9+0.3 made at 4.86 GHz with the VLA are presented, and compared with earlier observations at 1.49 GHz which hav…
Magnetohydrodynamic Models for the Structure of Pulsar-Wind Nebulae
Stephen P. Reynolds
The Crab Nebula is well-described at optical wavelengths and above by a steady-state magnetohydrodynamic model due to Kennel and Coroniti (1984). Can this class of model describe o…
Detecting X-ray Synchrotron Emission in Supernova Remnants: Implications for Abundances and Cosmic Rays
Kristy K. Dyer, Stephen P. Reynolds, Kazik J. Borkowski +1
The 10^51 ergs released in a supernova have far reaching consequences in the galaxy, determining elemental abundances, accelerating cosmic rays, and affecting the makeup of the int…
Low Frequency Insights Into Supernova Remnants
Kristy K. Dyer, Stephen P. Reynolds, Kazik J. Borkowski
Low frequency observations at 330 and 74 MHz can provide new insights into supernova remnants (SNR). We can test theoretical predictions for spectral index variations. Nonlinear mo…
Shock Acceleration and Gamma-Ray Emitting Supernova Remnants
Matthew G. Baring, Donald C. Ellison, Stephen P. Reynolds +2
Diffusive shock acceleration in the environs of a remnant's expanding shell is a popular candidate for the origin of SNR gamma-rays. In this paper, results from our study of non-li…