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The variable energy-distribution of the gamma-ray emission from Geminga
DOI: 10.1016/0273-1177(91)90158-G Bibcode: 1991AdSpR..11h.107G

Grenier, I. A.; Hermsen, W.; Hote, C.

The gamma-ray emission of Geminga during five COS-B observations has been analysed to derive its spectral properties between 50 MeV and 5 GeV. In all observations but one, the spectrum presents a turnover between 100 and 200 MeV, the source becoming very weak at the lowest gamma- ray energies. During the remaining observation, the spectrum is cons…

1991 Advances in Space Research
COS-B 7