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Fig. 2


Radial velocities of HD 206267Aa1 (filled circles) and HD 206267Aa2 (open circles). The left panel shows the RVs corresponding to our new measurements (Table 3), assuming a period of 3.710534 days, while the right panel showsour measurements along with those taken by Stickland (1995) and Burkholder et al. (1997), assuming a period of 3.709777 days. The solid and dashed lines indicate the orbital solution from Table 5.

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