Abstract
A new source of high velocity molecular gas to the south of the HII region NGC 2068 (M78) near the Herbig-Haro objects HH 25–26 is reported. The redshifted and blueshifted CO wings seen in this region are spatially separated indicating that this is another region of bi-polar mass outflow from a young stellar object. We compare this region to the other known regions of bi-polar mass outflow and discuss the implications of these energetic outflows.
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© 1982 D. Reidel Publishing Company
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Snell, R.L., Edwards, S. (1982). High Velocity Gas in Molecular Clouds. In: Roger, R.S., Dewdney, P.E. (eds) Regions of Recent Star Formation. Astrophysics and Space Science Library, vol 93. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7778-5_18
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DOI: https://doi.org/10.1007/978-94-009-7778-5_18
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-7780-8
Online ISBN: 978-94-009-7778-5
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