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[vsnet-campaign-dn 2069] SX LMi: relatively rapid fading?



SX LMi: relatively rapid fading?

    The Kyoto team performed time-series photometry of SX LMi and 
found that the object faded with the rate of 0.25 mag/day.  
This is somewhat faster compared with the ordinary superoutburst.  
In the light curve, we can find a hint of weak double-peaked variations 
in one orbital (~superhump) period, but they are not conclusive 
because the short base-line.  Tonight observation will also essential 
to reveal the nature of the current outburst.

Regards,
Makoto Uemura

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