You do not have permission to delete messages in this group
Copy link
Report message
Show original message
Either email addresses are anonymous for this group or you need the view member email addresses permission to view the original message
to bhtomt...@googlegroups.com, Przemek Mikołajczyk
Dear BHTOM Observers,
Some time in mid-October, the next EE Cephei eclipse will begin. It should take more or less two months. This star is very interesting for a variety of different reasons. Multiband photometry will be greatly appreciated, during, before and after the eclipse. EE Cep is now well visible throughout the entire night. The depth is hard to predict because it depends on the orientation/structure of the dark precessing disk. Historically, EE Cep’s eclipses have ranged roughly 0.6–2.0 mag in V. For context, the 2014 eclipse ended up being ~0.71 mag (V) - much shallower than expected - illustrating the uncertainty in advance forecasts.