Comparison of rotation period, chromospheric emission log _RHK, coronal emission log L_X/L_bol, and Li EW of HD 206893 to those of the Hyades (red symbols) and Pleiades (blue symbols) open clusters. In the first panel (rotation period), the filled circle shows the photometric period and the triangle the upper limit derived from the projected rotational velocity. In the same panel the continuous and dashed lines are the sequences of slow rotators for Pleiades and Praesepe, respectively (Stauffer et al. 2016). They overlap at the colour of HD 206893. The last two panels show the kinematic parameters of HD 206893 and those of several young moving groups. In these panels, the dashed box represent the locus of the Nearby Young Population as defined in Zuckerman et al. (2004). The dotted contours in the U vs. V plot mark the locus of kinematically young stars, as proposed by Montes et al. (2001).