Volume 372, Number 2, June III 2001
|Page(s)||L33 - L36|
|Published online||15 June 2001|
Discovery of a molecular outflow, near-infrared jet and HH objects towards IRAS 06047-1117
Centro de Astronomia e Astrofísica da Universidade de Lisboa, Observatório Astronómico de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal e-mail: firstname.lastname@example.org, email@example.com
2 Institute for Astrophysical Research, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA e-mail: firstname.lastname@example.org
3 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany e-mail: email@example.com, firstname.lastname@example.org
4 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany e-mail: email@example.com, firstname.lastname@example.org
Corresponding author: J. Yun, email@example.com
Accepted: 5 March 2001
We report discovery of a new young stellar object driving a point-symmetric, near-infrared jet and molecular outflow. The YSO is associated with IRAS 06047-1117 and is embedded in a dense molecular cloud core located southeast of Orion A. The jet is seen in the H2 line at 2.12 μm and extends over a total length of about ~0.4 pc. The driving source is optically invisible and has near-infrared colors and a spectral energy distribution consistent with a Class I source with an estimated luminosity of 6 . Two Herbig-Haro objects are seen in Hα images located close to the positions of maximum H2 emission.
Key words: infrared: stars / ISM: clouds / ISM: individual (IRAS 06047 / 1117) / ISM: jets and outflows / stars: formation / stars: mass-loss
© ESO, 2001
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