𝔖 Bobbio Scriptorium
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The gamma-ray observatory mission objectives and its significance for gamma-ray astronomy

✍ Scribed by D.L. Bertsch


Publisher
Elsevier Science
Year
1984
Tongue
English
Weight
718 KB
Volume
3
Category
Article
ISSN
0273-1177

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Very high energy Ξ³-rays at TeV energies so far have been detected from pulsar nebula, supernova remnants and active galactic nuclei, and explained by the emission of the electron and positron progenitor. The copious production of the energetic, nonthermal electrons and positrons generally implies an