I agree with Arne that CW Mon is probably _not_ another CG CMa. The AC2000 position is based on only a single image (usually there are three) taken during outvurst, but it was still near the limit (B ~12) of the AC plates. The fourth source I found recently is by Carlos Lopez in IBVS 2837, which contains positions derived from San Juan (Argentina) plates for several dwarf novae. For CW Mon he gives: 6 34 20.72 +00 04 52.9 (B1950) ...based on an SAO reference net. Our precession utility, which uses modern constants (i.e. not strictly a B-to-J conversion) gives: 6 36 54.50 +00 02 17.4 (J2000) ...which is again a bit north of the DWS97 spot. In any case, I think we've got this one nailed down pretty well. \Brian