Abstract
We present near-IR images of the shocked gas in in HH 167 (the LkHα234 jet) and HH 103. The H2 1-0 S(1) (2.122µm) and the 1.644µm [FeII] lines were observed. The relative spatial distribution of these two lines provides some insight into the nature of the shocks producing the objects.
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Schultz, A.S.B., Rank, D., Temi, P. et al. Shocked molecular hydrogen in the LkHα234 region. Astrophys Space Sci 233, 71–74 (1995). https://doi.org/10.1007/BF00627335
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DOI: https://doi.org/10.1007/BF00627335