Volume 458, Number 2, November I 2006
|Page(s)||L21 - L24|
|Published online||12 September 2006|
Letter to the Editor
A small jet in Chamaeleon I powered by a low-luminosity source
European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany e-mail: email@example.com
2 Institute for Astronomy, University of Hawaii, 640 N. Aohoku Place, Hilo, HI 96720, USA e-mail: firstname.lastname@example.org
Accepted: 6 September 2006
We report the discovery of a small bipolar Herbig-Haro jet, HH 872, powered by the low-luminosity source ESO-Hα 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 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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