Development of jets, outflows and HH objects

Details Development of jets, outflows and HH objects Development of jets, outflows and HH objects

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..515r&link_type=abstract

Highlights of Astronomy, Volume 15, p. 515-516

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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