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Keywords

ISM: Jets and outflows
Stars: Mass loss
Stars: Pre-main sequence

How to Cite

Entrainment in Herbig-Haro Objects. (2003). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 15(1), 115-119. https://astronomia.unam.mx/journals/rmxac/article/view/2003rmxac..15..115r
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Abstract

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.