Molecular mixing layers in stellar outflows

descriptionPublicationkeyboard_double_arrow_right Article , Part of book or chapter of book 01 Jan 1995 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 233, pages 139-144 (issn: 0004-640X, eissn: 1572-946X,

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Authors: S. D. Taylor; A. C. Raga;

doi: 10.1007/bf00627341 , 10.1007/978-94-009-1624-1_17

Molecular mixing layers in stellar outflows

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Abstract

High velocity jets from young stars interact with the surrounding molecular environment and molecular outflows quite possibly are the result. This interaction can take place through the formation of a turbulent mixing layer. Models have been constructed (following Cant/’o and Raga) of a plane mixing layer in the boundary between a high velocity, atomic wind (i.e., the stellar jet) and a stationary, molecular environment, computed considering a detailed chemical network.

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