600/800mm - 24" (1/25/14): at 375x, VV 123B appeared moderately bright, small, round, compact, 20" diameter, high surface brightness. VV 123A, situated just 25" S (nucleus of the Ring component) was cleanly resolved and appeared very faint, very small, round, 12" diameter, low surface brightness. The actual ring, extending south, was not seen.

900/1200mm - 48" (4/6/13): Arp 141 is an unusual interacting system, listed as a Ring galaxy with collider in Madore, Nelson and Petrillo's 2009 "Atlas and Catalog of Collisional Ring Galaxies". At the north end is VV 123B = Madore C1 (collider), which appeared bright, fairly small, round, 20" diameter, sharply concentrated with a very bright nucleus. This is the brightest component in the system. At the south edge of VV 123B (25" S of center) is VV 123A = Madore RN (Ring nucleus), which appeared fairly faint, small, irregularly round, 15" diameter. The ring component extends south of VV 123A and appeared as a faint, moderately large, oval haze, ~60"x30", mostly evident as a brighter arc or tail along the west side. This arc extends about as far south as a mag 14 star which is 1.5' SSW of VV 123B, though VV 123C, a small knot at the south end, was not resolved. Viewed at 488x and 610x.