[vsnet-alert 613] EG Cnc for IAUC

[Katsura Matsumoto <katsura@quasar.cc.osaka-kyoiku.ac.jp>]

I had submitted the following article to IAUC.

EG CANCRI
     K. Matsumoto, Osaka Kyoiku University, Japan, reports: "We obtained 
continuous CCD V-band light curves of EG Cnc on Dec. 2.625-2.791 UT and 
Dec. 3.625-3.708 UT with a 51-cm reflector at Osaka Kyoiku University. 
The observed light curves revealed suprehumps with a low (0.03-0.04 mag) 
amplitude. A preliminary analysis for combined light curves yielded a 
period of 0.0582 day, which is one of the shortest known among dwarf novae. 
The long interval (last ouburst: Nov. 1977) and large amplitude (more than 
7 mag) of outbursts, together with the short superhump period, support the 
WZ Sge-type classification of EG Cnc."


With best wishes,
Katsura Matsumoto (Osaka Kyoiku University, Japan)

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