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[vsnet-alert 5153] SY Vol still bright
- Date: Fri, 28 Jul 2000 17:50:05 +0900 (JST)
- To: vsnet-alert, vsnet-campaign
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 5153] SY Vol still bright
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
SY Vol still bright
The likely large-amplitude dwarf nova SY Vol is still bright according
to observations by Rod Stubbings. If this star is an SU UMa-type dwarf nova,
the present outburst should be a superoutburst. Time-resolved photometry
is very strongly encouraged. Follow-up information will be provided
in vsnet-campaign and vsnet-campaign-dn.
YYYYMMDD(UT) mag observer
20000723.492 142 (R. Stubbings)
20000723.533 142 (R. Stubbings)
20000724.514 140 (R. Stubbings)
20000724.551 140 (R. Stubbings)
20000724.585 140 (R. Stubbings)
20000727.480 144 (R. Stubbings)
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp