The kinematics of HH 34 from HST images with a nine-year time baseline

We study archival HST [S II ] 6716+30 and Hα images of the HH 34 outflow, taken in 1998.71 and in 2007.83. The 9 yr time baseline and the high angular resolution of these observations allow us to carry out a detailed proper-motion study. We determine the proper motions of the substructure of the HH...

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Main Authors: Raga, Alejandro C. (Author) , Lora, Verónica (Author)
Format: Article (Journal)
Language:English
Published: 2012 April 1
In: The astrophysical journal
Year: 2012, Volume: 748, Issue: 2
ISSN:1538-4357
DOI:10.1088/0004-637X/748/2/103
Online Access:Verlag, Volltext: http://dx.doi.org/10.1088/0004-637X/748/2/103
Verlag, Volltext: http://stacks.iop.org/0004-637X/748/i=2/a=103
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Author Notes:A.C. Raga, A. Noriega-Crespo, A. Rodríguez-González, V. Lora, K.R. Stapelfeldt, and S.J. Carey

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520 |a We study archival HST [S II ] 6716+30 and Hα images of the HH 34 outflow, taken in 1998.71 and in 2007.83. The 9 yr time baseline and the high angular resolution of these observations allow us to carry out a detailed proper-motion study. We determine the proper motions of the substructure of the HH 34S bow shock (from the [S II ] and Hα frames) and of the aligned knots within 30” from the outflow source (only from the [S II ] frames). We find that the present-day motions of the knots along the HH 34 jet are approximately ballistic, and that these motions directly imply the formation of a major mass concentration in 900 yr, at a position similar to the one of the present-day HH 34S bow shock. In other words, we find that the knots along the HH 34 jet will merge to form a more massive structure, possibly resembling HH 34S. 
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