ever found, 3C 75 is notable for having not one but two radio jets, each spewing from a separate nucleus. The two streamers run through the galaxy’s center, appear- ing to merge on the right. 
    The 3C 75 jets possess an interesting arcing structure, not typical of galaxy radio emissions. Within the galaxy, the emission is confined to a narrow profile and straight path, but on the left, at what is roughly the galaxy’s edge, the narrow jets expand into fat streams that bend sharply. On the right, the jets merge, continuing as a single entity, which, like those on the galaxy’s opposite side, widens and bends.
    The factors affecting the move- ment of radio jets are not well understood and are the focus of