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Paper: Detection of the γ-ray emission from the X-Ray nova GRO J0422+32
Volume: 261, The Physics of Cataclysmic Variables and Related Objects
Page: 637
Authors: Iyudin, A. F.; Haberl, F.
Abstract: The evolution of the γ-ray emission from GRO J0422+32 was followed by COMPTEL since its discovery outburst of August 1992 till August 1997, and for 3 observations preceding the nova outburst. It was found that the GRO J0422+32 γ-ray emission is mostly confined to the energies between 1.5 and 2.0 MeV. This emission is prominent during observations that correspond to phases between 0.0 and 0.5 of the nova ~120 day periodical activity.
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