A new southern star-formation region, located at an estimated distance of ~1.5 kpc in the Lynds 1664 dark cloud in Canis Major, is described. Lynds 1664 contains several compact star clusters, small stellar groups, and young stars associated with reflection nebulae. Narrow-band H{\alpha} and [SII] images obtained with 4-m CTIO telescope reveal more than 20 new Herbig-Haro objects associated with several protostellar outflows.
@article{arxiv.1604.08374,
title = {A new star-forming region in Canis Major},
author = {T. Yu. Magakian and T. A. Movsessian and J. Bally},
journal= {arXiv preprint arXiv:1604.08374},
year = {2016}
}