Abstract
It is now generally accepted that energetic, and often bipolar, mass outflows are an important phase in early stellar evolution. Evidence for such outflows is provided by a variety of phenomena. The most important ones are:
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(1)
the high-velocity molecular gas (HVMG)
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(2)
Herbig-Haro (HH) objects and optical jets.
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© 1988 Kluwer Academic Publishers
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Mundt, R. (1988). Collimated Outflows from Young Stars. In: Bianchi, L., Gilmozzi, R. (eds) Mass Outflows from Stars and Galactic Nuclei. Astrophysics and Space Science Library, vol 142. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2941-8_11
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DOI: https://doi.org/10.1007/978-94-009-2941-8_11
Publisher Name: Springer, Dordrecht
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