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Fig. 1


Radial velocities of HD 17505Aa1 (filled circles) and HD 17505Aa2 (open circles), assuming a period of 8.5690 days. The left panel shows the RVs corresponding to the new measurements (Table 2), while the right panel shows the solution obtained by combining our measurements with those of Hillwig et al. (2006). The solid and dashed lines indicate the orbital solutions from Table 4.

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