A narrow, bright feature associated with several types of astronomical object. Jets are seen mainly at radio but occasionally at other wavelengths. They emerge from the core of certain active galaxies and may extend for many hundreds of kiloparsecs. In some sources, notably radio galaxies, jets are commonly seen on both sides of the nucleus (double-sided jet) while in others, such as quasars, only one jet is normally seen (single-sided jet). Some jets exhibit the phenomenon of superluminal velocity. Optical stellar jets are seen emerging from young stars such as T Tauri stars and FU Orionis stars, and are associated with Herbig–Haro objects. The X-ray binary system SS433 has two jets.