Interstellar Gas and Star Formation Near the Peculiar Radio Galaxy NGC   4410A
  We present new multi-wavelength data for the NGC 4410 galaxy group. This group contains the peculiar radio galaxy NGC 4410A, which has a distorted double-lobed radio structure. NGC 4410A is strongly interacting with three nearby galaxies, and has a peculiar ring-like optical morphology, a number of luminous H II regions, as well as as tidal tails and bridges variously visible in optical, HI, and X-ray light. The gravitational interaction has affected the interstellar matter, the star formation rate, and the radio lobes in this system. 
Beverly J. Smith (East Tennessee State University), Megan Donahue   (Space Telescope Science Institute), and John Stocke (Un...