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[vsnet-campaign-dn 2081] SX LMi: again fading slowly
SX LMi: again fading slowly
The object again started the slow fading on January 30 on the basis
of our observation at Kyoto last night. The temporal state without
fading reported last night is probably caused by the beat phenomenon.
In the light curve on January 30, superhumps still exist, but decrease
in amplitude. The humps becomes smaller and wider, with a possible
second-hump feature. Period analysis of all data sets yields
0.069373(11) day, almost equal to that reported last night.
We are now observing SX LMi also tonight at Kyoto and confirmed
that it was still bright.
Regards,
Makoto Uemura
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
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