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Coupled stellar jet/molecular outflow models

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Abstract

Molecular outflows can be modelled as environmental material entrained into high velocity stellar jets. Even though models of this entrainment process are at this time quite uncertain, a few preliminary theoretical efforts have been made. Three different models are discussed, in which the molecular outflows are identified with the turbulent mixing layer at the edge of a jet, with a turbulent envelope (driven by a large number of internal working surfaces in the jet) and with the wake of one working surface.

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Raga, A.C. Coupled stellar jet/molecular outflow models. Astrophys Space Sci 216, 105–112 (1994). https://doi.org/10.1007/BF00982476

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