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WZ Sge: eclipse and superhump structure
Dear Colleagues,
The analysis of the Aug. 10-11 data (B. Martin, Kyoto, G. Masi)
using the same technique as in [vsnet-alert 6251] shows the persistence
of a shallow dip (0.04 mag) at the predicted phase of eclipses.
The hump features reported in [vsnet-alert 6251] have moved with
respect to the orbital phase -- they are not therefore associated with
the early superhumps, but are moving superhumps with complex multiple
peaks.
More detailed analysis is in progress.
Regards,
Taichi Kato
VSNET Collaboration team
Return to the Powerful Daisaku
vsnet-adm@kusastro.kyoto-u.ac.jp
