[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[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
- Delivered-To: vsnet-campaign-dn-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
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
Return to Home Page
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
Powered by ooruri technology