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[vsnet-outburst 4875] CU Vel outburst: call for time-resolved photometry
- Date: Wed, 11 Dec 2002 09:42:40 +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 4875] CU Vel outburst: call for time-resolved photometry
- Sender: owner-vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp
CU Vel outburst: call for time-resolved photometry
As reported in [vsnet-outburst 4872], the SU UMa-type dwarf nova CU Vel
is in outburst.
===
CU Vel in outburst
VELCU 021210.507 108 Stu.RASNZ
VELCU 021210.521 108 Stu.RASNZ
Regards,
Rod Stubbings
===
Surprizingly, no solid publication exists on the superhump observation
of CU Vel. Although the present outburst may be yet premature to determine
its nature, the long lack of outbursts preceding this outburst may suggest
a superoutburst. Please make intensive time-series observations to
obtain the (potentially first) full coverage of an outburst of this object.
The generally adopted superhump period is 0.07999 d. This period would
be a good measure for the required minimal length (2-3 superhump periods)
of the nightly runs.
Regards,
Taichi Kato
VSNET Collaboration team
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