2016ApJ...817..148O

We present the results of high-resolution near-IR spectroscopy toward the multiple outflows around the Herbig Be star LkHα 234 using the Immersion Grating Infrared Spectrograph. Previous studies indicate that the region around LkHα 234 is complex, with several embedded young stellar objects and the outflows associated with them. In simultaneous H- and K-band spectra from HH 167, we detected 5 [Fe ii] and 14 H₂ emission lines. We revealed a new [Fe ii] jet driven by radio continuum source VLA 3B. Position-velocity diagrams of the H₂1-0 S(1) λ2.122 µm line show multiple velocity peaks. The kinematics may be explained by a geometrical bow shock model. We detected a component of H₂emission at the systemic velocity (V_LSR= -10.2 km/s) along the whole slit in all slit positions, which may arise from the ambient photodissociation region. Low-velocity gas dominates the molecular hydrogen emission from knots A and B in HH 167, which is close to the systemic velocity; [Fe ii] emission lines are detected farther from the systemic velocity, at V_LSR= -100–130 km/s. We infer that the H₂ emission arises from shocked gas entrained by a high-velocity outflow. Population diagrams of H₂lines imply that the gas is thermalized at a temperature of 2500-3000 K and the emission results from shock excitation.