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[vsnet-campaign-dn 3262] TU Tri: most likely SS Cyg star

Date: Mon, 6 Jan 2003 16:31:12 +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-campaign-dn 3262] TU Tri: most likely SS Cyg star
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TU Tri: most likely SS Cyg star

Dear Colleagues,

   We have mostly finished analyzing the January 4 data of TU Tri (4.5 hours,
by Torii-san, RIKEN).  The data do not apparently show superhumps, likely
indicating that this object is an SS Cyg-type dwarf nova.  An analysis of
Jan. 5 observation will soon be undertaken.

Regards,
Taichi Kato

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