George Herbig was performed at the Lick Observatory, joined then the staff of Lick designed the coudé spectrograph for 3-m telescope for the Shane. The object lies in a dense molecular star-forming region in the constellation of Orion. Any leftover material swirling around the newborn protostar. V1057 Cyg faded P Cyg structure in II lines in the IR Ca and Hα. Several SOFIN runs extended so that a search over a number of successive nights. These spectra show rapid night-to-night changes at Hα in the wind structure of FU Ori.
The equivalent width of the P Cyg absorption varied cyclically with phase stability with a period of 14.8 days. A period of 3.54 days varies also cyclically with a period of 3.54 days. No convincing dependence was found also that certain critical lines. The possibility is considered also that FUor eruptions. CCD photometry has been obtained for the young clusters. A distance of 1.2 kpc follows from 5146 cluster members from the photometry of several late-type IC. Optical photometry is available in the IC for 700 stars. A number of such interlopers have been identified on the basis of proper motion. An unusually low vsini is unexceptional except for an unusually low vsini. The IC formed in a dense foreground section of the molecular cloud.