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Searches for γ-Rays from the Crab Nebula and its Pulsar
1971
Symposium - International astronomical union
Preserved Fulltext
The Crab Nebula has been regarded as the most promising celestial object to investigate for the detection of γ-rays. γ-ray emission might be expected from either the synchrotron or the inverse Compton mechanism. Periodic γ-ray emission could come from the pulsar, but no theory has yet been developed for such objects. Searches for γ-rays from both the Crab Nebula and the Crab pulsar made by a number of groups are described. Limits have been set to the γ-ray emission from both objects which are
doi:10.1017/s007418090000718x
fatcat:doi4u3io3ndivkiv5gwsth3rqi