VLA observations of radio sources in interacting galaxy pairs in poor clusters

Observations of 16 radio sources in interacting galaxies in 14 poor clusters were made using the Very Large Array in the B configuration at λ 6 and 2 cm. These sources had been unresolved in earlier observations at λ 21 cm, and were chosen as a sample to determine which of three models for radio source formation actually pertains in interacting galaxies. From the analysis of this sample, the starburst model appears most successful, but the "central monster" model could pertain in some cases.