Coupled stellar jet/molecular outflow models

Details Coupled stellar jet/molecular outflow models Coupled stellar jet/molecular outflow models

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216..105r&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 105-112

Astronomy and Astrophysics

Astrophysics

5

Magnetohydrodynamic Flow, Mixing Layers (Fluids), Molecular Flow, Plasma Jets, Plasma Turbulence, Stellar Envelopes, Stellar Models, Stellar Winds, Turbulent Mixing, Entrainment, Molecular Clouds, Shock Waves

Scientific paper

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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