Fig. 9
Inclination vs. vsini. The solid lines indicate the period of 7.4 d (obtained from the RV analysis) and 17 d (a lower limit obtained from the inclination constraint). The hatched area marks the vsini constraint from the FEROS and HARPS spectra; the orange and red areas mark the constraints for disk inclination from Sipos et al. (2009) and Goto et al. (2011), respectively.
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