The Spectrum  by a Bare NSs is not necessarily a bb
n Strong (angle-dependent)  absorption for photons with energy comparable or lower than the plasma frequency.

n Strong absorption around the e- and ion cyclotron frequency.

n Below the plasma freq, one of the two modes may be non-propagating: a whistler. Whistlers have very large, divergent refractive index (Melrose, 1986).

n Appearance of cut-off energies and evanescent modes which can not propagate into the medium.

n  If the refractive index has large imaginary part : highly damped modes. 
They can not penetrate much below the surface (Jackson, 1975).
RESULTS: absorption features may or may not appear in the X-ray spectrum, depending on the model parameters (mainly on B).