Gamma-Ray Astrophysic: A New Look at the Universe
Jacob Trombka 1,
Carl Fichtel 2,
Jonathan Grindlay 3, and
Robert Hofstadter 4
1 Senior scientist at the Laboratory for Astronomy and Solar Physics, NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771
2 Chief scientist at the Laboratory for High Energy Astrophysics, NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771
3 Assistant professor of astronomy at the Center for Astrophysics, Harvard College Observatory, Smithsonian Astrophysical Observatory, Cambridge, Massachusetts 02138
4 Professor in the Physics Department, Stanford University, Stanford, California 94305
Progress in
-ray astronomy has been very encouraging in recent years. These observations provide the most direct means of studying the largest transfer of energy occurring in astrophysical processes: the dynamic effects of the energetic charged cosmic-ray particles, element synthesis, and particle acceleration. Gammaray astronomical observations also find important application in studies of the development of the planets from the primitive solar nebula and of the nature of high-energy processes in the sun's atmosphere and their relation to the basic problems of solar activity.