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[vsnet-campaign-dn 3970] V551 Sgr: growth time of the superhumps
- Date: Wed, 24 Sep 2003 20:07:24 +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 3970] V551 Sgr: growth time of the superhumps
- Cc: vsnet-gcvs@ooruri.kusastro.kyoto-u.ac.jp
- 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
V551 Sgr: growth time of the superhumps
Dear Colleagues,
The VSNET Collaboration has received Sep. 22 data from Berto Monard.
The data suggest that the superhumps were already present at the time
of Monard's second night observation. This finding looks consistent
with the presence of low-amplitude variation on his Sep. 21 data.
The growth time of the superhumps is not unusually long, probably
consistent with the observed superhump period. The observed evolution
of the superhumps more resembles the usual evolution of superhumps in
relatively short-period normal SU UMa-type dwarf nova rather than
unusual WZ Sge-like systems.
Regards,
Taichi Kato
VSNET Collaboration team

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