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Fig. 2.

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Evolution of wind-burst matching points in the parameter space (for model XRB-A). The colored dots represent matching points with a relative error of δ < 0.01. The color scale corresponds to the time since burst peak expansion. Both energy outflow, Ė, and mass outflow, , were normalized in terms of Eddington luminosity in the electron scattering case, LX (see text). A reference value for = 1018 g s−1 is indicated by a vertical red dashed line.

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