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[vsnet-alert 3173] V503 Cyg anomalously high outburst frequency
- Date: Thu, 1 Jul 1999 11:24:36 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 3173] V503 Cyg anomalously high outburst frequency
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
V503 Cyg anomalously high outburst frequency
The SU UMa-type dwarf nova V503 Cyg (previously known as the short
supercycle system, Ts=89d Tn=30d) seems to be undergoing an extremely
enhanced outburst activeity state. Recent observations suggest outbursts
May 25 (Poyner, mv=14.5), Jun. 8 (Poyner, mv=15.3),
Jun. 11 (McKenna, mv=14.4), Jun. 19 (Muyllaert, mv=14.4).
Observations are encouraged to see whether the star has changed its
outburst properties, and whether the known superhump nature has changed.
YYMMDD(UT) mag observer
990615.028 <150 (G. Poyner)
990616.007 <142 (E. Muyllaert)
990616.047 <146 (G. Poyner)
990617.042 <146 (G. Poyner)
990618.067 <146 (G. Poyner)
990619.016 144 (E. Muyllaert)
990619.022 143 (G. Poyner)
990621.983 <142 (E. Muyllaert)
990622.008 <152 (G. Poyner)
990624.997 <142 (E. Muyllaert)
990630.005 144 (G. Poyner)
Regards,
Taichi Kato
Return to Daisaku Nogami
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