V725 Aql: August normal outburst
As reported by M. Simonsen and by G. Poyner, and confirmed by C. Jones,
an SU UMa-type dwarf nova, V725 Aql began an outburst on August 8.
The orbital period of V725 Aql estimated from the superhump period is
located at the middle of the period gap (2.5 hr)
The Ouda observing team reported on August 9 that the object was apparently
fainter than the 14.0 mag comparison star
This observation suggested this outburst to be a normal one, however
the object have not completely faded on August 11 (14.7:mag by C. P. Jones)
The fading from an outburst was confirmed in
( <14.7mag on August 12 by R. J. Modic).