[vsnet-outburst 9830] AQ Eri: superhump period

[Taichi Kato]

AQ Eri: superhump period

   Nakajima-san and Kiyota-san have reported further observations.
The superhump period determined from two nights' data was 0.06226(3) d.
Judging from the behavior up to now, the object may have undergone
a precursor outburst at the time of Stubbings's and ASAS detection.
The present superhumps were already present during the rising branch
from the temporary fading from the supposed precursor.

  YYYYMMDD(UT)   mag  observer
  20081222.1704 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20081225.1536 13.127V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20081225.547   132  (Rod Stubbings)
  20081226.523  13.78C  (Seiichiro Kiyota)
  20081226.599  13.51C  (Kazuhiro Nakajima)
  20081227.574  13.10C  (Kazuhiro Nakajima)

  Further observations are continuously needed to clarify the period
variation of the superhumps.