[vsnet-outburst 9196] ASAS002511+1217.2 possible brightening?

Taichi Kato tkato at kusastro.kyoto-u.ac.jp
Wed Jul 16 10:38:15 JST 2008


   According to ASAS-3 data, ASAS002511+1217.2 may be brighter than usual.
Although this detection may have been a noise, an examination of the field
might be useful.  The object is a WZ Sge-like dwarf nova which underwent
an superoutburst in 2004.

  YYYYMMDD(UT)   mag  observer
  20080629.4017 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080703.3913 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080707.3806 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080714.3940 16.380V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))


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