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[vsnet-campaign-dn 1170] WZ Sge: eclipse and superhump structure
- Date: Sat, 11 Aug 2001 14:59:57 +0900 (JST)
- To: vsnet-alert, vsnet-campaign-dn, vsnet-superoutburst
- From: Taichi Kato <tkato>
- Subject: [vsnet-campaign-dn 1170] WZ Sge: eclipse and superhump structure
- Sender: owner-vsnet-campaign-dn@kusastro.kyoto-u.ac.jp
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
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
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