Wind inhibition by X-ray irradiation in HMXBs: the influence of clumping and the final X-ray luminosity

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Fig. 10.

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Accretion X-ray luminosity according to Eq. (18) as a function of irradiation X-ray luminosity for the model 300-1 (black lines). Labels denote binary separation D. The intersections of straight red line, which denotes one-to-one relation, with black curves correspond to the solution of Eq. (18).

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