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[vsnet-chat 220] supercycle of V1113 Cyg
- Date: Wed, 16 Apr 1997 10:41:20 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 220] supercycle of V1113 Cyg
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Thanks to intensive monitoring by visual observers, the cycle lengths
of V1113 Cyg seem to have become pretty well established.
Recent outbursts:
JD (+2400000) mag type observers
---------------------------------------------------------
49597-612 13.3 super SNO,POY
49826-830 13.7 super POY,VAN,Wor,BRO
49893-895 13.9 normal VAN,BRO,PIE,POY
49956-959 13.8 normal JEN,VAN,BRO,POY,PIE
50025-036 13.5 super PIE,VAN,BRO,POY
50203-211 13.6 super POY,JEN,VAN
50280-282 13.8 normal PIE,BRO,POY,Kat
50308 14.0 normal? POY (single obs.)
50333-334 13.9 normal POY,BRO
50372-378 13.7 super POY,PIE,VAN,JEN
50420 13.9 normal? POY (single obs.)
50546 14.0 super POY,SNO,JEN
Intervals between adjacent superoutbursts are 229, 199, 178, 169, 174
d (shortening of supercycle?), average of recent three ones being 170 d.
This system seems to be rather peculiar in that normal outbursts are
rather infrequent compared to numerous superoutbursts. Systems with only
two (or three) normal outbursts in one supercycle is rarely met in such
short supercycle (170 d) SU UMa-type dwarf novae (cf. Warner B. 1995,
ApSS, 226, 187). From the viewpoint of the outburst pattern, there may
be some resemblance to the recently discovered peculiar SU UMa-type dwarf
nova V503 Cyg. Close monitoring to confirm the cycle length of normal
outbursts is desirable than ever.
Regards,
Taichi Kato
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