TeV gamma ray burst from SN 1987 A

Details TeV gamma ray burst from SN 1987 A TeV gamma ray burst from SN 1987 A

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...268..607a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 268, no. 2, p. 607, 608.

Astronomy and Astrophysics

Astrophysics

Gamma Ray Bursts, Supernova 1987A, Compton Effect, Electron Scattering, High Energy Electrons

Scientific paper

The TeV gamma ray burst observed from SN 1987A was explained by Schlickeiser and Stanev (1991) as due to Compton scattering of X-rays from high energy electrons in the Klein-Nishina limit. It is shown here that Compton scattering of infrared and optical photons from the nebula reduces the required energy in the electrons by several orders of magnitude.

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