| Abstract | Aperture synthesis observations of H I in Arp 205 are described. The spatial resolution is 1.9 x 2.4 arcmin, and the velocity resolution 32 km/s. The maps show H I in rotation about the dwarf galaxy UGC 6016 and independently about NGC 3448. Other H I emission to the west of NGC 3448 and with a smaller recession velocity is indicative that NGC 3448 is a disturbed system. Radio continuum observations of the nuclear source in NGC 3448 are presented at 151, 408, 1407, 1417 and 2700 MHz. The orgin of the disruption observed in this system is discussed in relation to tidal interactions, and the possibility of two distinct systems along the same line of sight. |
