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Figure 1: Evolution of plasma temperature A), density B), pressure C), and velocity D) distributions along the flux tube from the chromosphere to the unperturbed accretion stream, sampled every 60 s from 0 to 300 s ( left panels) and every 30 s from 330 to 420 s ( right panels). The figure shows the inner portion of the spatial domain, including the chromosphere and the hot slab. |
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Figure 2: Observed X-ray spectrum of the star MP Mus (gray line) with the synthetic spectrum derived from the simulation (black line). |
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