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A&A 458, L21-L24 (2006)
DOI: 10.1051/0004-6361:20066161
Letter
A small jet in Chamaeleon I powered by a low-luminosity source
F. Comerón1 and B. Reipurth21 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany
e-mail: fcomeron@eso.org
2 Institute for Astronomy, University of Hawaii, 640 N. Aohoku Place, Hilo, HI 96720, USA
e-mail: reipurth@ifa.hawaii.edu
(Received 1 August 2006 / Accepted 6 September 2006)
Abstract
We report the discovery of a small bipolar Herbig-Haro
jet, HH 872, powered by the low-luminosity source
ESO-H
574 in Chamaeleon I. The end-to-end projected size
of the jet in [SII] images is only 3150 AU. Infrared images
marginally resolve the central source showing a structure
elongated perpendicularly to the jet axis, possibly a disk seen at
a large angle with respect to the plane of the sky. The brightest
feature of the jet, peaking at a distance of 1''6 from the
central source, is likely to result from enhanced outflow activity
in the last decade.
Key words: stars: low-mass, brown dwarfs -- stars: pre-main sequence -- ISM: jets and outflows
© ESO 2006
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