[vsnet-alert 3530] V725 Aql superhump detection

[Makoto Uemura <uemura@kusastro.kyoto-u.ac.jp>]

V725 Aql superhump detection

  From our observation on 26 and 27 Sep. at Kyoto, we detected 
the superhump of V725 Aql, which is undergoing the outburst 
([vsnet-alert 3505]), and confirmed that V725 Aql is SU UMa-type 
dwarf nova and this outburst is superoutburst. 

  We performed period analysis using the phase dispersion minimization (PDM)
method, yielding 0.109 d or 0.123 d as the candidates. 
There is possibility that V725 Aql has a period within the period gap 
from this result. 

  V725 Aql is keeping this superoutburst now.
Observers are strongly urged to obtain more accurate period of superhump.
We wish some collaborations.

Regards,
Makoto Uemura, Taichi Kato

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