[vsnet-outburst 8010] V344 Lyr very likely superoutburst

[Taichi Kato]

   The current outburst of V344 Lyr is most likely a superoutburst.
Nakajima-san's observation on Aug 28 show brightening trend and
likely superhumps.  The profile of the humps was unusual (slower rise
and faster decline).  These observations may suggest that the
superhumps are just growing now.
The last likely superoutburst was in 2007 May.  If both two outbursts
are confirmed to be genuine superoutbursts, the supercycle is as
short as 101 d (not inconsistent with earlier research).
For a discussion, see MNRAS 2002, 53 (astro-ph/0110317).

  YYYYMMDD(UT)   mag  observer
  20070811.634  <181CR  (Hiroyuki Maehara)
  20070812.617  <173C  (Hiroyuki Maehara)
  20070812.956  <156  (Gary Poyner)
  20070823.980  <148  (Gary Poyner)
  20070824.925  <153  (Gary Poyner)
  20070825.926  <148  (Gary Poyner)
  20070826.860  15.33CR  (Maciej Reszelski)
  20070826.939   149  (Gary Poyner)
  20070827.490  15.33C  (Kazuhiro Nakajima)
  20070828.551  14.93C  (Kazuhiro Nakajima)