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[vsnet-campaign 785] TV Crv clear superhumps
- Date: Wed, 21 Feb 2001 20:55:23 +0900 (JST)
- To: vsnet-alert, vsnet-campaign, vsnet-superoutburst
- From: Taichi Kato <tkato>
- Subject: [vsnet-campaign 785] TV Crv clear superhumps
- Sender: owner-vsnet-campaign@kusastro.kyoto-u.ac.jp
TV Crv clear superhumps
Dear Colleagues,
The Kyoto observation on Feb. 20 (Uemura et al.) of TV Crv has shown
extremely clear, fully developed superhumps. The best superhump period
is 0.0649 d, which confirms the previous esimate (0.0650 d, Howell et al.).
This finding confirms that TV Crv is one of short orbital period systems.
The present excellent visibility will allow us to precisely determine
the superhump period and its change, as well as the full development of
outburst and hump structures. More detailed analysis will be presented
by Uemura-san et al.
More observations are strongly requested!
Regards,
VSNET Collaboration team
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
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