New, high-resolution, near-infrared observations of HH1

Davis, C.J., Smith, M.D., Eisloffel, J. (2000) New, high-resolution, near-infrared observations of HH1. Monthly Notices of the Royal Astronomical Society, 318 (3). pp. 747-752. ISSN 0035-8711. (doi:10.1046/j.1365-8711.2000.03766.x) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:50137)

The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided.
Official URL: http://dx.doi.org/10.1046/j.1365-8711.2000.03766.x

Abstract

We present new, high-resolution, near-infrared images of the HH 1 jet and bow shock. H2 and [Fe II] images are combined to trace excitation changes along the jet and across the many shock features in this flow. Echelle spectra of H2 profiles towards a few locations in HH 1 are also discussed. Gas excitation in oblique, planar C-type shocks best explains the observations, although J-type shocks must be responsible for the observed [Fe II] emission features. Clearly, no single shock model can account for all of the observations. This will probably be true of most, if not all, Herbig-Haro flows.

Item Type:	Article
DOI/Identification number:	10.1046/j.1365-8711.2000.03766.x
Uncontrolled keywords:	Circumstellar matter, Infrared: ISM: lines and bands, Infrared: stars, ISM: individual: HH 1, ISM: jets and outflows, ISM: kinematics and dynamics
Subjects:	Q Science > QB Astronomy > QB460 Astrophysics
Divisions:	Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User:	Giles Tarver
Date Deposited:	11 Aug 2015 10:17 UTC
Last Modified:	05 Nov 2024 10:35 UTC
Resource URI:	https://kar.kent.ac.uk/id/eprint/50137 (The current URI for this page, for reference purposes)

University of Kent Author Information

Smith, M.D..

Creator's ORCID:	https://orcid.org/0000-0002-4289-5952
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