High energy gamma-ray photons are the prime probes of the relativistic or high-energy universe, populated by black holes, neutron stars, supernovae, quasars, and matter-antimatter annihilations. Through studying the gamma-ray sky, astrophysicists are able to better understand the formation and behav
Very High Energy Gamma Ray Astronomy
โ Scribed by Weekes T.
- Year
- 2003
- Tongue
- English
- Leaves
- 238
- Category
- Library
No coin nor oath required. For personal study only.
โฆ Synopsis
Weekes (Whipple Observatory, Harvard-Smithsonian Center for Astrophysics) summarizes the status of gamma-ray astronomy at energies above 30 MeV at a critical point in the development of the discipline: the hiatus between the demise of the Energetic Gamma Ray Experiment Telescope telescope, and the launch of the next generation of space telescope, GLAST, and the completion of the next generation of imaging atmospheric Cherenkov detectors involving large arrays of telescopes. He discusses detectors, telescopes in space, the galactic plane, observations of the Crab Nebula, gamma-ray pulsars and binaries, unidentified sources, gamma-ray bursts, diffuse background radiation, and other topics. Distributed in the US by AIDC.
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