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We present a high-resolution, near-IR spectroscopic study of multipleoutflows in the LkH$\alpha$ 234 star formation region using the ImmersionGRating INfrared Spectrometer (IGRINS). Spectral mapping over the blueshiftedemission of HH 167 allowed us to distinguish at least three separate, spatiallyoverlapped, outflows in H${_2}$ and [Fe II] emission. We show that the H${_2}$emission represents not a single jet, but complex multiple outflows driven bythree known embedded sources: MM1, VLA 2, and VLA 3. There is a redshiftedH${_2}$ outflow at a low velocity, $\VLSR$ $<$ $+$50 {\kms}, with respect tothe systemic velocity of $\VLSR$ $=$ $-$11.5 {\kms}, that coincides with theH${_2}$O masers seen in earlier radio observations two arcseconds southwest ofVLA 2. We found that the previously detected [Fe II] jet with $|$$\VLSR$$|$ $>$100 {\kms} driven by VLA 3B is also detected in H${_2}$ emission, and confirmthat this jet has a position angle about 240$\degree$. Spectra of theredshifted knots at 14$\arcsec$$-$65$\arcsec$ northeast of LkH$\alpha$ 234 arepresented for the first time. These spectra also provide clues to the existenceof multiple outflows. We detected high-velocity (50$-$120 {\kms}) H${_2}$ gasin the multiple outflows around LkH$\alpha$ 234. Since these gases move atspeeds well over the dissociation velocity ($>$ 40 {\kms}), the emission mustoriginate from the jet itself rather than H${_2}$ gas in the ambient medium.Also, position-velocity diagrams and excitation diagram indicate that emissionfrom knot C in HH 167 come from two different phenomena, shocks andphotodissociation.

High-resolution near-IR Spectral mapping with H$_{2}$ and [Fe II] lines of Multiple Outflows around LkH$\alpha$ 234