From owner-vsnet-adm@kusastro.kyoto-u.ac.jp Fri May 29 06:10 JST 1998 Date: Thu, 28 May 1998 23:08:52 +0200 From: Liza van Zyl <vanzyl@uctvms.uct.ac.za> Subject: (No Subject in original) Dear VS Net persons: I have been looking at your announcement of the supposed superoutburst of V2051 Oph. If you look at my paper in MNRAS Vol 224, p.733,1987 you will see that I did some high speed photometry of V2501 in outburst and that (a) it is probably too small an amplitude to be a superoutburst and (b) there are no superhumps. The eclipse centred on a "superhump" shown on your Web page is just the enhanced orbital hump that appears during outburst, I do not understand just what is going on during an outburst of V2501; I hope that more extensive coverage will provide some clues. With best wishes, Brian Warner (in the middle of a two week observing run at the observatory at Sutherland, devoted entirely to GW Lib).