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[vsnet-campaign-dn 3462] GZ Cnc observation from Nyrola team
- Date: Fri, 21 Feb 2003 20:05:14 +0900 (JST)
- To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp,vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-campaign-dn 3462] GZ Cnc observation from Nyrola team
- Delivered-To: vsnet-campaign-dn-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
GZ Cnc observation from Nyrola team
Dear Colleagues,
The light curve of GZ Cnc (Feb. 20) from the Nyrola team shows clear
presence of intermediate-period (around 40 min) variations. The profile
even looks "minature" superhumps (the same feature was also observed
by the Kyoto team and Greg Bolt during a past outburst). There is no
indicatation of the presence of short-period flare-like oscillations.
Regards,
Taichi Kato
VSNET Collaboration team
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