Abstract
Recent CO(3-2) observations of the bipolar outflow of the large Herbig-Haro complex HH 111 are presented. Molecular emission is found to be co-extensive with the marked optical jet within one arcminute of the central object, and exhibits either acceleration or velocity sorting. The results for the HH 111 field are contrasted with those for the HH 34 region, which was observed also during the same program.
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© 1993 Springer Science+Business Media Dordrecht
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Matthews, H.E., Hayashi, S.S., Dent, W.R.F., Davis, C.J. (1993). Submillimetre Observations of HH 111 with the JCMT. In: Errico, L., Vittone, A.A. (eds) Stellar Jets and Bipolar Outflows. Astrophysics and Space Science Library, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1924-5_5
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DOI: https://doi.org/10.1007/978-94-011-1924-5_5
Publisher Name: Springer, Dordrecht
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