Entrainment in Herbig-Haro Objects

Details Entrainment in Herbig-Haro Objects Entrainment in Herbig-Haro Objects

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..115r&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

3

Ism: Jets And Outflows, Stars: Mass Loss, Stars: Pre-Main Sequence

Scientific paper

This paper first reviews the literature of entrainment of molecular material into HH jets. The available models can, in principle, reproduce the H[2] emission of a number of HH objects. However, there are some HH jets with aligned knots which show basically identical structures in the H[2] and atomic/ionic line emission. For these objects, we suggest a possible interpretation in terms of the ablation of molecular gas from dense clumps which are immersed within the jet beam.

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