Abstract
This paper reviews various hydrodynamical models proposed for explaining bipolar molecular outflows from young stars. The different possibilities discussed are: wind-driven molecular shells, steady state filled flows, and jet-driven bow shocks. Particular emphasis is placed on comparisons between model predictions and observations of molecular flows. While it appears that jet-driven bow shocks are at the present time the most popular mechanism for explaining molecular outflows, other models have interesting characteristics that might be relevant for at least some objects.
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Cabrit, S., Raga, A., Gueth, F. (1997). Models of Bipolar Molecular Outflows. In: Reipurth, B., Bertout, C. (eds) Herbig-Haro Flows and the Birth of Low Mass Stars. International Astronomical Union / Union Astronomique Internationale, vol 182. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5608-0_15
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DOI: https://doi.org/10.1007/978-94-011-5608-0_15
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