Fig. 5
Predicted energy fluxes of 1 TeV photons from PSR B1259−63 corresponding to the three different non-radiative loss profiles as shown in Fig. 4 compared to the 2004 (black dots) and 2007 (red empty squares) HESS data. The vertical grey boxes indicate the location of the stellar disc. The vertical dashed and dotted lines denote the position of the stellar equatorial plane (Bogomazov 2005).
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