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KV Dra: superhump period
We have reduced the last night observation at Kyoto.
Using combined data sets kindly sent from all collaborators,
we performed period analysis and calculate the best superhump
period to be 0.059948(27) d. This is slightly shorter than that
reported during the previous superoutburst.
Time-series observations are encouraged to study the evolution
of superhumps. The Kyoto team started tonight run at 10:50 (UT) Sep. 3.
The object is still in superoutburst.
Regards,
Makoto Uemura
on behalf of VSNET Collaboration team
Return to the Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
