Particle acceleration and Tycho's supernova remnant.
Abstract
Particle acceleration in shock waves may be very efficient at converting bulk kinetic energy into energy density in high-energy particles. The author investigates the implications for the dynamics and evolution of a Sedov-type blast wave, with particular reference to determining the energy of the supernova event associated with Tycho's supernova remnant. He finds that X-ray and radio observations favour a low efficiency of conversion of kinetic energy to high-energy particles, a supernova explosion energy of about 8×1043J, and an ambient density of about 4 atom cm-3.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- November 1984
- DOI:
- Bibcode:
- 1984MNRAS.211..195H
- Keywords:
-
- Particle Acceleration;
- Supernova Remnants;
- Boundary Value Problems;
- Flow Equations;
- Radio Astronomy;
- Shock Waves;
- Two Fluid Models;
- X Ray Astronomy;
- Astrophysics