The entrainment of molecular material through a mixing layer along the walls of a HH jet beam has been modeled analytically (Cantó & Raga 1991; Stahler 1994) and numerically (Taylor & Raga 1995; Lim et al . 1999). However, when full radiative jet simulations are carried out, the molecular, environmental material remains within a dense shell which follows the shape of the leading bow shock. Because of this, no molecular material reaches the outer boundary of the jet beam, and therefore no “side-entrainment” of molecular gas into the fast jet beam takes place.
CITATION STYLE
Raga, A. C., López-Cámara, D., Cantó, J., Esquivel, A., Rodríguez-González, A., & Velázquez, P. F. (2009). Development of jets, outflows and HH objects. Proceedings of the International Astronomical Union, 5(H15), 515–516. https://doi.org/10.1017/s1743921310010458
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