Comprehensive UV and optical spectral analysis of Cygnus X-1 - Stellar and wind parameters, abundances, and evolutionary implications

Open Access

Fig. 11

Same as Fig. 10 but IUE observations at orbital phase ϕ ∼ 0 during low-hard state are shown. We adopted a lower X-ray luminosity L_{_X} ∼ 3--5 × 10³⁶ erg s⁻¹ in the model. Adopted wind parameters in models are shown in legend.

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