“…These estimates may, however, be affected by observational selection, since the distance to DR 15 is substantially greater than that to Lk Hα 101 (about 707 pc) [25] and even more so than that to the cluster IC 348 (about 300 pc) [24]. On the other hand, several Herbig-Haro objects, which form substantially extended flows [1], have been found in the group of T Tau stars. In the meantime, no directed flows have been detected in the regions of Lk Hα 101 and IC 348, even though they are at smaller distances.…”