On evidence for quasi-parallel and quasi-perpendicular acceleration in supernova remnants

Details On evidence for quasi-parallel and quasi-perpendicular acceleration in supernova remnants On evidence for quasi-parallel and quasi-perpendicular acceleration in supernova remnants

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...338..963l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 338, March 15, 1989, p. 963-971.

Astronomy and Astrophysics

Astrophysics

5

Interstellar Magnetic Fields, Limb Brightening, Particle Acceleration, Stellar Coronas, Supernova Remnants, Brightness Distribution, Line Of Sight, Milky Way Galaxy, Morphology

Scientific paper

An attempt is made to determine whether or not the structure of supernova remnant shells is dependent on the angle between the line of sight and the Galactic magnetic field and if this structure can be explained either by quasi-parallel or quasi-perpendicular acceleration. The method used to determine the line of sight angles to the magnetic field is described. A model for the emissivity of a supernova remnant is developed.

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