Results of the integral-field spectroscopy of the young binary Haro 6-10 sh
ow the presence of an emission Herbig-Haro jet, superposed on the bright re
flection nebula. Length of the jet is only 5", its position angle is 195 de
grees, radial velocity changes from -30 to - 80 km s(-1). On the base of th
ese observations and of the existing polarimetric and infrared data the nor
thern (infrared) component of the Haro 6-10 system is suggested as a probab
le source of the out-flow.