I have received the following message from Rafael Costero, and forward this with the permission of him and cited observers (via Costero). Observations (though very difficult) right now are very critical in understanding the current, extremely rare, fading episode of this unique binary planetary nebula nucleus. Any attempts are highly appreciated. Regards, Taichi Kato -------------------------------------------------------------------------- From costero@astroscu.unam.mx Wed Jul 30 15:38 JST 1997 Date: Wed, 30 Jul 97 01:40:04 CST Subject: V651 Mon V651 Mon is now barely observable in the (cold) morning twilight (for those brave observers in the southern hemisphere). In spite of extremely difficult observing conditions, a few admirable observers secured some estimates before the object became truly unobservable in late May and mid-June, and again are now doing their best, weather permitting. They have recently obtained four very valuable estimates of the object. I consider their measurements very much worth being known by vsnet members, so asked for their consent to share the data with your organization, thanks to which I learned of the current occultation episodes on this interesting object (or are they over?). Their estimates are listed below: V651 Mon (Last two months) Date Mag. Observer YYMMDD(UT) (vis) Code ___________________________________ 970529.701 <13.2 JAN 970530.701 <13.2 JAN 970530.384 <14.4 Stu 970602.389 12.0 Stu 970602.701 12.8: JAN 970603.361 12.0 Stu 970604.363 11.8: Stu 970605.369 11.2 Stu ! 970606.360 11.3 Stu 970607.363 11.3 Stu 970608.351 11.5 Stu 970608.379 11.6 Far 970610.343 12.5: Stu !! 970615.347 <13.2 Stu !!! 970617.344 12.0 Stu !! 970618.348 11.8 Stu 970619.349 11.4 Stu 970620.347 11.2 Stu 970622.358 11.2 Stu ! ------------------------------------ 970723.775 11.0: Jo 970724.769 11.2 Jo 970724.840 11.4 Stu 970725.772 11.3 Jo Key to observers: Far: Fraser Farrell Jo: Albert Jones JAN: Jan Hers Stu: Rod Stubbings Weather in Australian and New Zealander mornings has prevented any further estimates since July 25. It is very important to know if occultations are still going on. My guess is that, if so, the object should be weaker than mag 12 or so any time between July 27 and August 5, or during all that time interval. I'm sure you will understand the importance to have at least one estimate during these days. Sure it's hard, the object beeing so close to the Sun; it is, I am sure, imposible for us northeners. But I call again for your very valuable help for the case of this very interesting object. With the moon now waning and comet Hale-Bopp not far from V651 Mon (about 12 degrees south and 10 min further east), the early-rising might worth the effort! I am very much endebted to all those observers that had already tried and, in many occations, obtanied the valuable observations needed to know the nature of the occulting dust-cloud passing in front of V651 Mon, the ~16-day period, spectroscopic binary central star of the planetary nebula NGC 2346. With my deep gratitude to you and all vsnet-ers, Rafael Costero Instituto de Astronomia, UNAM P.O. Box 70-264 04510 Mexico, D.F. costero@astroscu.unam.mx