Fig. 5
Left panel: SB2 orbital solution for the WR binary in AB 6 (WR: black curve; O: green curve) using the complete set of RV measurements of the He II λ4686 line for star A and the He Iλ4471 line for star B (see legend). Right panel: same as left panel, but using the N V λλ4604, 4620 doublet RVsfor star A. See text for details.
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