Fig. 13.
Simulated X-ray emission emanating from accretion column modeled in run D5e10-B30-A45, as a function of the height above the star surface (z), for three cases: without any local absorption effect (black continuous line), and with the local absorption integrating the emission from the right (green dashed line) and from the left (red dotted line) side of the accretion stream.
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