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Interpretation of the light curve of gamma-ray emission from the 2021 outburst of the recurrent nova RS Ophiuchi
Nova outbursts take place in binary star systems comprising a white dwarf and either a low-mass Sun-like star (classical novae) or, a red giant. GeV gamma-ray emission has been detected from a dozen classical novae and from one nova in a symbiotic system (V407 Cyg) by Fermi-LAT. For classical novae, …