Observational tests of particle acceleration theory - Shell supernova remnants

Details Observational tests of particle acceleration theory - Shell supernova remnants Observational tests of particle acceleration theory - Shell supernova remnants

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..264..195a&link_type=abstract

In: Particle acceleration in cosmic plasmas; Proceedings of the Workshop, Bartol Research Inst., Newark, DE, Dec. 4-6, 1991 (A93

Astronomy and Astrophysics

Astrophysics

Galactic Cosmic Rays, Particle Acceleration, Particle Theory, Stellar Envelopes, Supernova Remnants, Brightness Distribution, Radio Observation, Relativistic Particles

Scientific paper

Ways in which radio continuum observations of shell SNR can be applied to the study of astrophysical particle acceleration are discussed. As an example, radio observations of SNRs Cas A, G39.2-0.3, and G41.1-0.3 are presented. It is found that spatial variations in the radio spectral index, observed in several shell remnants, in conjunction with measurements of radio brightness and polarization, can provide constraints for various acceleration models.

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