Herbig-Haro jet in the Haro 6-10 system

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Stars: Pre-Main Sequence, Ism: Herbig-Haro Objects, Ism: Individual Objects: Haro 6-10, Ism: Jets And Outflows

Scientific paper

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 arcsec, its position angle is 195degr , 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. Based on observations taken at the Special Astrophysical Observatory, Russia

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