Fig. 2.

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Origin of emission seen across the Brackett γ line. The contribution of individual images to the total line flux is indicated on the central image showing the line profile. The brightness maps are in units of the maximum emission. The emission of the stellar surface is saturated. Orange to red colours indicate the regions of maximum emission. The system is seen at an inclination of 30° and an rotational phase of ∼0.25, similarly to Fig. 1.
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