Fig. 13
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Mass-loss rate per unit area as a function of distance to the star. Left: different times (from light to dark blue with increasing time) for our fiducial model compared to those from Picogna et al. (2021) for the same stellar mass and X-ray spectrum (black). Right: comparing the fiducial model (dark blue) with those where we switch off certain areas of microphysics in order to test their impact.
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