ULTRA HIGH ENERGY γ-FLUX FROM SUPERNOVA 1987a

21 November 1987

journal article
Published by World Scientific Pub Co Pte Ltd in Modern Physics Letters A

Vol. 2 (11) , 801-804
https://doi.org/10.1142/s0217732387001014

Abstract

High energy γ-ray from the SN 1987a in LMC will be observable by such a detection system as used for Cyg X-3, if it is installed in the southern hemisphere. The γ-ray flux will rise and decline in about one year and the maximum event rate could be 10⁴ times larger than Cyg X-3 in some model.

Keywords

FLUX
ENERGY
SUPERNOVA 1987A
ULTRA HIGH ENERGY

This publication has 0 references indexed in Scilit: