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Fig. 3

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Schematic view of the regions of dominance for various mechanisms of photon escape on the magnetic field – temperature plane, I – diffusion escape, II – relativistic jumps, III – natural line broadening, IV – recoil. The region where cyclotron driven wind is possible is above the dashed lines. The left figure is for a white dwarf (MWD = 1   M), and the right figure is for a neutron star (MNS = 1.4   M, R = 12 km).

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