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[vsnet-campaign 47] BZ UMa

Dear colleagues,

aprox. 4.8 hours long run on BZ UMa in R-band Kroun-Cousins filter using
SBIG ST-7 and 0.4m Newtonian telescope shows rapid decline form current
outburst which seems to be a normal one. The rate of decline is
aproximately 0.66 mag / day. The limit of possible fast variability was
equal to 0.05mag and there is no flickering up to this limit.

this mean it's impossible to be an SU UMa type variable in
superoutburst.
Let's observe some different one :)

Regards

Rudolf Novak
N. Copernicus Observatory Brno

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