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Fig. 5.

image

Integrated TeV light curves (E >  1 TeV) with comparisons of observations. The observational data are taken from the preliminary data reported by Romoli et al. (2017). The dashed and dotted lines correspond to the IC scattering with seed photons from the star and the shock heating of the disc. The solid line represents the total flux with both components. The dash-dotted line shows the effect of the disc matter clump at the shock front on TeV emissions.

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