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Astron. Astrophys. 347, 266-271 (1999)

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Herbig-Haro jet in the Haro 6-10 system *

T.A. Movsessian and T.Yu. Magakian

Byurakan Astrophysical Observatory, 378433 Aragatsotn reg., Armenia (tigmov@bao.sci.am; tigmag@sci.am)

Received 13 January 1998 / Accepted 29 March 1999

Abstract

Results of the integral-field spectroscopy of the young binary Haro 6-10 show the presence of an emission Herbig-Haro jet, superposed on the bright reflection nebula. Length of the jet is only 5", its position angle is 195o, radial velocity changes from -30 to -80 km s-1. On the base of these observations and of the existing polarimetric and infrared data the northern (infrared) component of the Haro 6-10 system is suggested as a probable source of the outflow.

Key words: stars: pre-main sequence – ISM: Herbig-Haro objects – ISM: individual objects: Haro 6 – 10 – ISM: jets and outflows

* Based on observations taken at the Special Astrophysical Observatory, Russia

Send offprint requests to: T.A. Movsessian

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© European Southern Observatory (ESO) 1999

Online publication: June 18, 1999
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