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Fig. 7.


Spectra of the rotating NS with the parameters M′ = 1.519 M, Re = 15.48 km, and ν* = 700 Hz computed for two inclination angles i= 0° (blue solid curve) and i= 90° (red solid curves), and for two relative luminosities (same over the surface) ℓ= 0.9 (top panel) and ℓ= 0.1 (bottom panel). The solid curves represent spectra computed taking accurate local spectra for atmosphere models from Suleimanov et al. (2012). The dashed curves correspond to the diluted blackbody approximation of the local spectra. Solar chemical composition of the atmosphere is assumed.

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