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Fig. 3


Gray-scale representation of the low-resolution spectrophotometry of 29 November 1995 collected into 11 phase bins and repeated for 1.64 orbits. Left: observed spectra with the bin containing φ = 0 remaining empty. Center: cyclotron spectra obtained by subtracting the dM4e secondary star and the underlying continuum. Right: model of the cyclotron line emission for a field strength of 31.8 MG (see text).

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