Gamma-Ray Sources is a class of astronomical objects or phenomena that emit electromagnetic radiation predominantly in the gamma-ray energy range, distinguished from other radiative sources by the extreme physical processes—such as cosmic ray interactions, relativistic particle acceleration, or nuclear transitions—that produce photons typically above 100 keV.
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BATSE observations of gamma-ray burst spectra. I - Spectral diversity
D. L. Band, J. L. Matteson, Linda Ford et al. · The Astrophysical Journal · 1993 · 2.3K citations
Natural Sciences, Astronomy, Physics +12
An unusual supernova in the error box of the γ-ray burst of 25 April 1998
T. J. Galama, P. M. Vreeswijk, J. van Paradijs et al. · Nature · 1998 · 1.9K citations · Full text
Natural Sciences, Astronomy, Physics +14
The physics of gamma-ray bursts
Tsvi Piran · Reviews of Modern Physics · 2005 · 1.8K citations · Full text
Natural Sciences, Astronomy, Physics +12
The Supernova–Gamma-Ray Burst Connection
S. E. Woosley, J. S. Bloom · Annual Review of Astronomy and Astrophysics · 2006 · 1.8K citations · Full text
Natural Sciences, Astronomy, Physics +12
The Third EGRET Catalog of High-Energy Gamma-Ray Sources
P. Sreekumar, S. D. Hunter, P. L. Nolan et al. · NASA Technical Reports Server (NASA) · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +14
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