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[vsnet-campaign-dn 3752] V803 Cen superhumps
- Date: Sat, 7 Jun 2003 14:23:39 +0900 (JST)
- To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp,vsnet-superoutburst@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-campaign-dn 3752] V803 Cen superhumps
- 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
V803 Cen superhumps
Dear Colleagues,
We have received a nice data set from Neil D Butterworth. The light curve
clearly indicate the presence of 0.06 mag superhumps. The period determined
from this observation is 0.01860(8) d, which agrees with the "nominal
superhump period" of this system within errors. The profile is placed at:
http://vsnet.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/V803_Cen/sh0306.gif
Although the light curve may look slightly noisy, mainly because of
the low amplitude of the variations, the presence of the superhump-type
variation is secure.
Regards,
Taichi Kato
VSNET Collaboration team
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