The impact of thermal winds on the outburst lightcurves of black hole X-ray binaries

Open Access

Fig. 4.

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Same as Fig. 3 except that 𝒞 is calculated self-consistently from scattering in the wind (bottom panel, solid line). Top panel: grey solid line shows Ṁ_in for a non-irradiated disc, with wind mass loss taken into account. All other line codes as in Fig. 3.

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