X-ray irradiation of the stellar wind in HMXBs with B supergiants: Implications for ULXs

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Fig. 1

Radial variations of velocity in the model 150-60 without clumping with the total X-ray luminosity L_X = 10³⁷ erg s⁻¹ (left panel) and L_X = 10⁴¹ erg s⁻¹ (right panel). Individual curves are labeled by a binary separation D in units of R_⊙.

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