Abstract
Preliminary results of a search for high velocity CO in relatively nearby (d<3kpc) star forming cloud cores are presented. Detailed CO, CS, and VLA observations of the molecular outflow region associated with NGC 2071 suggest that a disk constrained stellar wind is responsible for the bipolar high velocity CO flow.
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© 1982 D. Reidel Publishing Company
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Bally, J. (1982). High Velocity CO Line Wings and the Dynamics of Star Forming Molecular Cloud Cores. 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_37
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DOI: https://doi.org/10.1007/978-94-009-7778-5_37
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-7780-8
Online ISBN: 978-94-009-7778-5
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