[Aavso-photometry] new nova

[Aaron Price]

 According to Wolfgang's latest post, this is likely associated with a 
blue progenitor so is likely a dwarf nova. So if anyone is imaging tonight 
try to go for time series for as long as possible to look for superhumping 
behavior. If this is a dwarf nova, then it is likely a UGWZ and so early 
superhump behavior is important to monitor as it can change phase and help 
confirm the classification.

-- 
Aaron Price (PAH), Technical Assistant, Technology
American Association of Variable Star Observers
http://www.aavso.org