Expected X-ray emission from SN 1987A - Analytical consideration

Details Expected X-ray emission from SN 1987A - Analytical consideration Expected X-ray emission from SN 1987A - Analytical consideration

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13.1042g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Dec. 1987, p. 1042-1054. In Russian. In Russian. In Russian.

Statistics

Computation

6

Computational Astrophysics, Emission Spectra, Supernovae, X Ray Spectra, Compton Effect, Electron Scattering, Photoabsorption, Spectral Energy Distribution, Stellar Envelopes

Scientific paper

In terms of diffusion (for the space) and Fokker-Planck (for photon energy) approximations a fast converging series describing the supernova envelope hard X-ray emission (hν < 1 MeV) was obtained assuming the central source of hard photons of any type. Compton scattering on cold electrons follwed by the recoil effect and photoabsorption are the main processes which determine the spectrum's shape. An opportunity of envelope geometry investigation during the observations of direct emission γ-quanta is also considered.

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