Protostars and Planets VI, Heidelberg, July 15-20, 2013

Poster 1K060

Turbulent Entrainment Model of Molecular Outflows

Li, Guang-Xing (MPIfR Bonn)
Qiu, Keping (Nanjing University)
Wyrowski, Friedrich (MPIfR Bonn)
Menten, Karl (MPIfR Bonn)

Protostellar outflow is a prominent process accompanying the formation of stars. It is generally agreed that wide-angled protostellar outflows come from the interaction between the wind from a forming star and the ambient gas. However, how the interaction takes place is unclear. In this work, we theoretically investigate the possibility that the outflow results from interaction between the wind and the ambient gas in the form of turbulent entrainment. Unlike previous models, turbulent motion of the ambient gas around the protostar is taken into account. In our model, the ram-pressure of the wind balances the turbulent ram-pressure of the ambient gas, and the outflow consists of the ambient gas entrained by the wind. The calculated outflow from our modelling exhibits a conical shape. The total mass of the outflow is determined by the turbulent velocity of the envelope as well as the outflow age, and the velocity of the outflow is several times larger than the velocity dispersion of the ambient gas. The outflow opening angle increases with the strength of the wind and decreases with the increasing ambient gas turbulence. The outflow exhibits a broad line width at every position. We propose that the turbulent entrainment process, which happens ubiquitously in nature, plays a universal role in shaping protostellar outflows.

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