Volume 523, November-December 2010
|Number of page(s)||10|
|Section||Interstellar and circumstellar matter|
|Published online||10 November 2010|
Departament d’Astronomia i Meteorologia (IEEC-UB), Institut de
Cièncias del Cosmos, Universitat de Barcelona, Martí i Franquès 1, 08028
e-mail: email@example.com; firstname.lastname@example.org
2 Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
3 Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Spain
4 GTC Office, Spain
5 Instituto Astrofísica Andalucía, CSIC, Camino Bajo de Huétor 50, 18008 Granada, Spain
Accepted: 2 August 2010
Context. The dark cloud Lynds 723 (L723) is a low-mass star-forming region where one of the few known cases of a quadrupolar CO outflow has been reported. Two recent works have found that the radio continuum source VLA 2, towards the centre of the CO outflow, is actually a multiple system of young stellar objects (YSOs). Several line-emission nebulae that lie projected on the east-west CO outflow were detected in narrow-band Hα and [S ii] images. The spectra of the knots are characteristic of shock-excited gas (Herbig-Haro spectra), with supersonic blueshifted velocities, which suggests an optical outflow also powered by the VLA 2 YSO system of L723.
Aims. Our aim is to study L723 in the near-infrared and look for line-emission nebulae associated with the optical and CO outflows.
Methods. We imaged a field of ~5′ × 5′ centred on HH 223, which includes the whole region of the quadrupolar CO outflow with narrow-band filters centred on the [Fe ii] 1.644 μm and H2 2.122 μm lines, together with off-line Hc and Kc filters. The [Fe ii] and H2 line-emission structures were identified after extracting the continuum contribution, if any. Their positions were determined from an accurate astrometry of the images.
Results. The H2 line-emission structures appear distributed over a region of ′̣ (~0.5 pc for a distance of 300 pc) at both sides of the VLA 2 YSO system, with an S-shape morphology, and are projected onto the east-west CO outflow. Most of them were resolved in smaller knotty substructures. The [Fe ii] emission only appears associated with HH 223. An additional nebular emission from the continuum in Hc and Kc appears associated with HH 223-K1, the structure closest to the VLA 2 YSO system, and could be tracing the cavity walls.
Conclusions. We propose that the H2 structures form part of a large-scale near-infrared outflow, which is also associated with the VLA 2 YSO system. The current data do not allow us to discern which of the YSOs of VLA 2 is powering this large scale optical/near-infrared outflow.
Key words: stars: formation / Herbig-Haro objects / infrared: ISM / ISM: jets and outflows
Based on observations made with LIRIS at the 4.2 m Williams Herschel Telescope operated at the Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias.
Fits files of Table 1 are available at CDS via anonymous ftp to cdsarc.u-strasbg.fr (126.96.36.199) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/523/A16
© ESO, 2010
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