A possible explanation of the secular flattening of the spectrum of Cassiopeia A

Details A possible explanation of the secular flattening of the spectrum of Cassiopeia A A possible explanation of the secular flattening of the spectrum of Cassiopeia A

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56.1235f&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, Nov.-Dec. 1979, p. 1235-1243. In Russian.

Astronomy and Astrophysics

Astronomy

1

Cassiopeia A, Secular Variations, Stellar Spectra, Distribution Functions, Dynamic Stability, Electron Distribution, Electrostatic Waves, Flattening, Relativistic Particles, Stellar Evolution, Stellar Magnetic Fields, Supernovae, Wave Generation

Scientific paper

The effect of secular flattening of the Cassiopeia-A spectrum can be
accounted by means of the kinetic instability of the radiating electrons
relative to the Alfven waves. This instability is caused by the
decreasing of the magnetic field in the supernova shell.

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