Fig. 6
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Comparison of the intensity distribution of two images from Fig. 1 (− 8 and + 863 km s−1) with the intensity CLV of the stellar wind CMFGEN model. The model CLVs are convolved with a point spread function with 6 mas diameter to match the resolution of the observed images. Top: Brα stellar wind image of the primary star at the velocity of − 8 km s−1 and the corresponding CMFGEN model. Bottom: continuum + 863 km s−1 image of thestellar wind of the primary star and the corresponding CMFGEN model.
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