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Detection of a γ-ray burst of very long duration and very high energy

✍ Scribed by Hurley, K. ;Dingus, B. L. ;Mukherjee, R. ;Sreekumar, P. ;Kouveliotou, C. ;Meegan, C. ;Fishman, G. J. ;Band, D. ;Ford, L. ;Bertsch, D. ;Cline, T. ;Fichtel, C. ;Hartman, R. ;Hunter, S. ;Thompson, D. J. ;Kanbach, G. ;Mayer-Hasselwander, H. ;von Montigny, C. ;Sommer, M. ;Lin, Y. ;Nolan, P. ;Michelson, P. ;Kniffen, D. ;Mattox, J. ;Schneid, E. ;Boer, M. ;Niel, M.

Book ID
109791305
Publisher
Nature Publishing Group
Year
1995
Tongue
English
Weight
131 KB
Volume
374
Category
Article
ISSN
0028-0836

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✍ A. A. Stepanian 📂 Article 📅 1989 🏛 Springer Netherlands 🌐 English ⚖ 385 KB

The latest achievements in very high-energy (VHE) gamma-ray astronomy are discussed. Types of candidate objects for the sources of very high-energy gamma-quanta are considered, and pulsars, as the most probable ones, are anticipated. The objectives of VHE gamma-ray astronomy are presented, outlining