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Conference Summary: What is High Energy Astrophyics?

Published online by Cambridge University Press:  26 May 2016

Virginia Trimble*
Affiliation:
Department of Physics and Astronomy, University of California, Irvine, CA 92697, and Astronomy Department, University of Maryland, College Park, MD 20742, USA

Abstract

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The original intent of the conference was to focus, first, on the physical processes (accretion, collimation, and all the rest) shared by two or more of the kinds of sources generally thought of as belonging to high energy astrophysics and, second, on the full range of phenomena, at all wavelengths, exhibited by those sources. This summary therefore addresses some of these issues as well as some new results presented at the symposium and some of the still-unanswered questions that were raised.

Type
Part 11 Summing Up
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Baade, W. & Zwicky, F. 1934, PNAS, 20, 254 and 259 CrossRefGoogle Scholar
Bolton, C. T. 1972, Nat., 235, 271; Nat. Phys. Sci., 240, 124 CrossRefGoogle Scholar
Giacconi, R. et al. 1962, PRL, 9, 439 Google Scholar
Gratton, L. 1966, High Energy Astrophysics (Academic Press) p. 2 Google Scholar
Ho, C. et al. 1992, Gamma Ray Bursts (Cambridge University Press)Google Scholar
Novikov, I. D. & Zeldovich, Ya. B. 1966, Nuovo Cimento Suppl., 4, 810 Google Scholar
Salpeter, E. E. 1964, ApJ, 140, 796 CrossRefGoogle Scholar
Shklovskii, I. S. 1953, Dokl. Akad. Nauk SSSR, 91, 475 Google Scholar
Webster, B. L. & Murdin, P. 1972, Nat., 235, 37 Google Scholar
Wheeler, J. A. 1966, ARA&A, 4, 303 Google Scholar
Zeldovich, Ya. B. & Novikov, I. D. 1964, Sov. Phys. Dokl., 9, 834 Google Scholar