in MWSC at Galactic longitude $l = 289\deg$. Even the poorly populated cluster Feigelson 1 [also known as the $\epsilon$ Chameleontis group, @2013ApJS..209...26F] at $(l,b)=(300\deg,-15\deg)$ was found as one seed. Of the other seeds, the concentrations at $(l,b)=(300\deg,-1\deg)$ and the large group at $(l,b)=(297\deg,+8\deg)$ seemed to be the most interesting, because of their proximity to the Sun; the mean of the TGAS parallaxes of these groups were 9.5 and 9.1mas, respectively. We called the southern group Group A and the northern one Group B. The [violet diamond]{} in between Group A and B corresponds to the center of “Group 4" in @2017AJ....153..257O. Their group 4 actually comprises our groups A and B, and in their notation it has a size of 114 (number of stars in the group). It is worth mentioning that already @1997ESASP.402..545C found a moving group of 33 nearby A-type dwarfs at a mean distance of 105 pc at $(l,b) = (304\deg,+3\deg)$. For our Group A we determined the phase space coordinates on the basis of the TGAS positions, proper motions and parallaxes, as well as with radial velocities retrieved from SIMBAD, and found mean values of: [[ in the Barycentric equatorial coordinate system with the $\xi$-axis 