Double features in radio supernova remnants

Details Double features in radio supernova remnants Double features in radio supernova remnants

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..265p&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Apr. 1985, p. 265-270) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Mar.-Apr

Astronomy and Astrophysics

Astronomy

Radio Sources (Astronomy), Supernova Remnants, Entropy, Field Strength, Shock Wave Interaction, Synchrotron Radiation

Scientific paper

The two-component magnetic field perturbations that will develop after
passage of a shock wave may engender double strong-strong and
strong-weak features in the radio maps of old supernova remnants. The
distance separating the components provides an independent estimate of
the magnetic field direction and strength.

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