[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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