2018ApJ...858...23O

We present a high-resolution, near-IR spectroscopic study of multiple outflows in the LkHα 234 star formation region using the Immersion GRating INfrared Spectrometer (IGRINS). Spectral mapping over the blueshifted emission of HH 167 allowed us to distinguish at least three separate, spatially overlapped outflows in H₂ and [Fe II] emission. We show that the H₂ emission represents not a single jet but rather complex multiple outflows driven by three known embedded sources: MM1, VLA 2, and VLA 3. There is a redshifted H₂ outflow at a low velocity, V_LSR <+50 km s^–1, with respect to the systemic velocity of V_LSR = -11.5 km s^–1, that coincides with the H₂O masers seen in earlier radio observations 2'' southwest of VLA 2. We found that the previously detected [Fe II] jet with | V_LSR| > 100 km s^–1 driven by VLA 3B is also detected in H₂ emission and confirm that this jet has a position angle of about 240°. Spectra of the redshifted knots at 14''-65'' northeast of LkHα 234 are presented for the first time. These spectra also provide clues to the existence of multiple outflows. We detected high-velocity (50-120 km s^–1) H₂ gas in the multiple outflows around LkHα 234. Since these gases move at speeds well over the dissociation velocity (>40 km s^–1), the emission must originate from the jet itself rather than H₂ gas in the ambient medium. Also, position-velocity and excitation diagrams indicate that emission from knot C in HH 167 comes from two different phenomena, shocks and photodissociation.