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Fig. D.1
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Velocity dependence of the X-ray emissivity in CMFGEN for different onset velocities: υx/υ∞ = 5 % in red and υx/υ∞ = 70 % in blue. The black dotted horizontal line marks the point where −υ∞/υ(r) = 1. which can be physically interpreted as where the shocks in the wind would roughly become relevant to produce X-rays.
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