[vsnet-superoutburst 1728] SW UMa post-superoutburst behavior

[Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>]

SW UMa post-superoutburst behavior

Dear Colleagues,

   We have finished analyzing the Nov. 16 data from Tanabe-san (VSNET Okayama
Station).  We have also finished anlyzing the Kyoto Nov. 17 data.

   On Nov. 16, SW UMa seems to have become slightly brighter than on the
previous nights, breaking the slow declining trend.

   Short-term variations with time-scales of 10-20 min are strongly present.
Some of them seem to show some degree of conherence.  Some of the variations
look like to be associated with late superhumps and their harmonics.

   From these observation, SW UMa is confirmed to remain active.

Regards,
Taichi Kato
VSNET Collaboration team

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