Fig. 6
Local spectrum of a neutron star with magnetic field B = 1011 G, normal to the surface, and with effective temperatures Teff = 106 K, 5 × 105 K, and 2 × 105 K (marked near the curves). The partially ionized atmosphere spectrum (solid lines) is compared with the fully ionized atmosphere model (dashed lines) and with the nonmagnetic atmosphere model (dotted lines).
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