Entrainment in Herbig-Haro objects
This paper first reviews the literature of entrainment of molecular material into HH jets. The available models can, in principle, reproduce the H2 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/i...
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paper:paper_14052059_v15_n_p115_Raga2023-06-08T16:13:16Z Entrainment in Herbig-Haro objects Raga, Alejandro Velázquez, Pablo Fabián Mininni, Pablo Daniel ISM: Jets and outflows Stars: Mass loss Stars: Pre-main sequence This paper first reviews the literature of entrainment of molecular material into HH jets. The available models can, in principle, reproduce the H2 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. © Copyright 2003: Instituto de Astronomía, Universidad Nacional Autónoma de México. Fil:Raga, A.C. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Velázquez, P.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Mininni, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2003 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v15_n_p115_Raga http://hdl.handle.net/20.500.12110/paper_14052059_v15_n_p115_Raga |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
ISM: Jets and outflows Stars: Mass loss Stars: Pre-main sequence |
spellingShingle |
ISM: Jets and outflows Stars: Mass loss Stars: Pre-main sequence Raga, Alejandro Velázquez, Pablo Fabián Mininni, Pablo Daniel Entrainment in Herbig-Haro objects |
topic_facet |
ISM: Jets and outflows Stars: Mass loss Stars: Pre-main sequence |
description |
This paper first reviews the literature of entrainment of molecular material into HH jets. The available models can, in principle, reproduce the H2 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. © Copyright 2003: Instituto de Astronomía, Universidad Nacional Autónoma de México. |
author |
Raga, Alejandro Velázquez, Pablo Fabián Mininni, Pablo Daniel |
author_facet |
Raga, Alejandro Velázquez, Pablo Fabián Mininni, Pablo Daniel |
author_sort |
Raga, Alejandro |
title |
Entrainment in Herbig-Haro objects |
title_short |
Entrainment in Herbig-Haro objects |
title_full |
Entrainment in Herbig-Haro objects |
title_fullStr |
Entrainment in Herbig-Haro objects |
title_full_unstemmed |
Entrainment in Herbig-Haro objects |
title_sort |
entrainment in herbig-haro objects |
publishDate |
2003 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v15_n_p115_Raga http://hdl.handle.net/20.500.12110/paper_14052059_v15_n_p115_Raga |
work_keys_str_mv |
AT ragaalejandro entrainmentinherbigharoobjects AT velazquezpablofabian entrainmentinherbigharoobjects AT mininnipablodaniel entrainmentinherbigharoobjects |
_version_ |
1768542803166494720 |