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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…
Separating Thermal and Nonthermal X-Rays in Supernova Remnants I: Total Fits to SN 1006 AD
K. K. Dyer, S. P. Reynolds, K. J. Borkowski +2
The remnant of SN 1006 has an X-ray spectrum dominated by nonthermal emission, and pre-ASCA observations were well described by a synchrotron calculation with electron energies lim…
Thermal and Nonthermal X-Ray Emission in SNR RCW 86
K. J. Borkowski, J. Rho, S. P. Reynolds +1
Supernova remnants may exhibit both thermal and nonthermal X-ray emission. Such remnants can be distinguished by the weakness of their X-ray lines, because of the presence of a str…
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…
New Models for X-Ray Synchrotron Radiation from the Remnant of Supernova 1006 AD
K. K. Dyer, S. P. Reynolds, K. J. Borkowski
Galactic cosmic rays up to energies of around 10^15 eV are assumed to originate in supernova remnants (SNRs). The shock wave of a young SNR like SN 1006 AD can accelerate electrons…