EDP Sciences
Free Access
Volume 431, Number 1, February III 2005
Page(s) 223 - 234
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361:20041821
Published online 02 February 2005

A&A 431, 223-234 (2005)
DOI: 10.1051/0004-6361:20041821

The near-infrared excitation of the HH 211 protostellar outflow

B. O'Connell1, 2, M. D. Smith1, D. Froebrich3, C. J. Davis4 and J. Eislöffel5

1  Armagh Observatory, College Hill, Armagh BT61 9DG, Northern Ireland, UK
    e-mail: boc@arm.ac.uk
2  Physics Department, Trinity College Dublin, College Green, Dublin 2, Ireland
3  School of Cosmic Physics, Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
4  Joint Astronomy Centre, 660 N. A'ohoku Place, University Park, Hilo, Hawaii 96720, USA
5  Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenberg, Germany

(Received 10 August 2004 / Accepted 12 October 2004 )

The protostellar outflow HH 211 is of considerable interest since it is extremely young and highly collimated. Here, we explore the outflow through imaging and spectroscopy in the near-infrared to determine if there are further diagnostic signatures of youth. We confirm the detection of a near-infrared continuum of unknown origin. We propose that it is emitted by the driving millimeter source, escapes the core through tunnels, and illuminates features aligning the outflow. Narrow-band flux measurements of these features contain an unusually large amount of continuum emission. [FeII] emission at 1.644  $\mu$m has been detected and is restricted to isolated condensations. However, the characteristics of vibrational excitation of molecular hydrogen resemble those of older molecular outflows. We attempt to model the ordered structure of the western outflow as a series of shocks, finding that bow shocks with J-type dissociative apices and C-type flanks are consistent. Moreover, essentially the same conditions are predicted for all three bows except for a systematic reduction in speed and density with distance from the driving source. We find increased K-band extinctions in the bright regions as high as 2.9 mag and suggest that the bow shocks become visible where the outflow impacts on dense clumps of cloud material. We propose that the outflow is carved out by episodes of pulsating jets. The jets, driven by central explosive events, are responsible for excavating a central tunnel through which radiation temporarily penetrates.

Key words: ISM: jets and outflows -- stars: circumstellar matter -- infrared: ISM -- ISM: Herbig-Haro objects -- ISM: individual objects: HH 211

SIMBAD Objects

© ESO 2005

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.