Fig. 11
Skymaps of the emitted radiation as produced by a rapidly rotating oblate AMP with one or two antipodal spots. The star is taken to have Re = 15 km, M = 1.6 M⊙, and ν = 600 Hz. The spot sizes are ρ = 10°, and the emission is coming from an isotropic blackbody with Teff = 2 keV. The red curves enclose the area where occultation is observed.
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