W5 is an active region of star formation located at ∼ 1.9 kpc in the Perseus spiral arm within Cassiopeia. We have surveyed W5 in the optical (Hα, [S II], and i filters), and at 1.1 mm. Our surveys cover several square degrees. Several highly collimated stellar jets have been discovered, along with other interesting outflows and Herbig-Haro objects. We have obtained optical spectra with the ARC APO 3.5 m telescope at various position angles for several of these jets and outflows, revealing jet velocities of ∼ 200 km s − 1.
