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[vsnet-alert 1819] Superhump of V2051 Oph was detected
- Date: Tue, 26 May 1998 19:42:09 +0900
- To: vsnet-alert@kusastro.kyoto-u.ac.jp
- From: Seiichiro Kiyota <skiyota@abr.affrc.go.jp>
- Subject: [vsnet-alert 1819] Superhump of V2051 Oph was detected
- In-Reply-To: <199805260303.MAA28733@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear observers,
PDM analysis by Kato using CCD observation by Kiyota on May 20-22 (posted to vsnet-obs)
indicates that superhump period of V2051 Oph is around 0.0642d.
This period is a little bit longer than orbital (eclispse) period.
So, we conclude that V2051 is one of member of UGSU (SU UMa type).
Seiichiro Kiyota and Taichi Kato
----
Seiichiro Kiyota skiyota@abr.affrc.go.jp
Laboratory of Stress Physiology
Department of Plant Physiology
National Insititute of Agrobiological Resources
Tel:81-298-38-8384
Fax:81-298-38-8347
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