From owner-vsnet-obs@kusastro.kyoto-u.ac.jp Sun Dec 1 09:59:27 1996 X-Sender: tvanmuns@pophost.innet.be X-Mailer: Windows Eudora Light Version 1.5.2 Mime-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Date: Sun, 01 Dec 1996 02:17:39 -0100 To: observations@aavso.org, JBortle@aol.com, guy@tahq.demon.co.uk, tkato@kusastro.kyoto-u.ac.jp, gp@star.sr.bham.ac.uk, pvancaut@innet.be, bill.worraker@aea.orgn.uk, nogami@kusastro.kyoto-u.ac.jp, safnet@mesiob.obspm.fr, KFA02524@niftyserve.or.jp, vsnet-obs@kusastro.kyoto-u.ac.jp, NAH01147@niftyserve.or.jp, ebroens@innet.be, fidusz@alba.zpok.hu, sno@iris.elte.hu From: Tonny Vanmunster <tvanmuns@innet.be> X-Distribute: distribute [version 2.1 (Alpha) patchlevel=19] X-Sequence: vsnet-obs 4461 Subject: [vsnet-obs 4461] CVC 115 (EG Cnc) Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp BELGIAN ASTRONOMICAL SOCIETY V.V.S. - Working Group Variable Stars Cataclysmic Variables Circular No.115 1996, December 1 Ed.: T. Vanmunster, Walhostraat 1A, 3401 Landen, BELGIUM Internet: tvanmuns@innet.be TEL. 32-11-831504 =================================================================== EG Cnc [NL/UG:, 11.9v - 17:v] ============================= We have been informed by Patrick Schmeer, Germany about an outburst of EG Cnc. This most interesting object, called Huruhata's Variable, has been seen only once before (in November 1977). A confirmative visual observation has been made by Tonny Vanmunster, Belgium. Here are some details : 1996 Nov. 30.917 UT, 12.5 (P. Schmeer, 0.20-m SCT, Seq: GSC); Nov. 30.951 UT, 12.0 (P. Schmeer); Nov. 30.989 UT, 11.8 (P. Schmeer); Dec. 01.021 UT, 12.1 (T. Vanmunster, 0.35-m refl., seq: GSC); Given the long recurrence time of this object, it is most likely that this a UGWZ-type dwarf nova. Therefor, follow-up observations at each stage of the light curve are of utmost importance. Time series CCD photometry is highly encouraged. Tonny Vanmunster