Available formats: HTML | PDF | (gzipped) PostScript
Herbig-Haro jet in the Haro 6-10 system *
T.A. Movsessian and
Received 13 January 1998 / Accepted 29 March 1999
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
Send offprint requests to: T.A. Movsessian
Online publication: June 18, 1999