Fig. 10

X-ray images of the whole domain as seen by an observer with a line of sight of 45° with the equatorial plane. On the left column panels are soft X-ray [ 0.1−2.0 ]keV flux values, on the right hand side panels, hard X-ray [ 2.0−10 ]keV flux values. The flux values are computed assuming a distance of 500 pc and no interstellar absorption. The images refer to run F4f1.00a and are taken at the same times as those of Fig. 7.
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