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[vsnet-outburst 4909] BZ UMa: Vanmunster's obsevation
- Date: Sat, 21 Dec 2002 09:43:40 +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-outburst 4909] BZ UMa: Vanmunster's obsevation
- Sender: owner-vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp
BZ UMa: Vanmunster's obsevation
Dear Colleagues,
Tonny Vanmunster has kindly sent the BZ UMa data (vsnet-campaign-dn 3160).
We have confirmed Tonny's finding. The amplitude of variation related
to orbital (or superhump) period is an order of 0.01 mag, assuming the
reported period. Although the current outburst may be a normal outburst,
QPO-like signals were most prominent during the declining stage in the
past outbursts. Please keep this in mind and follow the evolution of
the current outburst.
Regards,
Taichi Kato
VSNET Collaboration team
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp