Abstract
In this paper the morphological and kinematical properties of jets and collimated “optical” flows from young stellar objects are reviewed. Numerous recently obtained high-quality CCD images are shown to illustrate the morphological properties of these flows and their associated bow-shock like structures. The currently available data on the jet sources are also reviewed. In addition to a few other topics (e.g. jet’s working surface and radiative bow shocks) the kinematic properties of the driving gas of molecular flows from low-mass stars are discussed. It is suggested that it consists mainly of neutral, atomic gas with velocities in the order of 50 km/s.
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Mundt, R. (1988). Flows and Jets from Young Stars. In: Dupree, A.K., Lago, M.T.V.T. (eds) Formation and Evolution of Low Mass Stars. NATO ASI Series, vol 241. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3037-7_16
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DOI: https://doi.org/10.1007/978-94-009-3037-7_16
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