Abstract
After summarizing the basic properties of molecular outflows, I discuss several important issues that have seen recent theoretical or observational advance, namely: the outflow structure and velocity field, implications of outflow energetics on the nature of proto-stellar winds, Extremely High Velocity neutral components, and the evolutionary status of outflow sources.
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Cabrit, S. (1993). Molecular Outflows from Young Stellar Objects. 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_1
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DOI: https://doi.org/10.1007/978-94-011-1924-5_1
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