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Fig. 7
Comparison of model spectra computed for two WD masses, 0.6 (thin curves) and 0.9 (thick curves) M⊙ and two relative magnetospheric radii, Rm/R = 2 (dashed curves) and 1000 (solid curves). The local mass accretion rate is fixed to a = 1 g s-1 cm-2 for all the computed spectral models.
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