Abstract
Results from studies of the extended Herbig-Haro flux HH 276 in the region of FS Tau A/B are presented. Long-slit and Fabry-Perot spectroscopy were carried out on the 6-m telescope at the Special Astrophysical Observatory of the Russian Academy of Sciences and the 2.6-m telescope at the Byurakan Astrophysical Observatory. A new Herbig-Haro knot HH 276E, located on the axis of the already known outflow HH 276, was discovered. The radial velocities of this outflow indicate that the flux is oriented perpendicular to the line of sight. A presumed source of the flux, a bright infrared object, has been found. The slit spectrum in the optical range confirms the youth of this object and reveals signs of a Herbig-Haro outflow.
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