[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-campaign-dn 3967] Re: V551 Sgr: drefinite superoutburst of a new SU UMa star!
- Date: Tue, 23 Sep 2003 20:01:53 +0900 (JST)
- To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp,vsnet-superoutburst@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-campaign-dn 3967] Re: V551 Sgr: drefinite superoutburst of a new SU UMa star!
- Cc: vsnet-gcvs@ooruri.kusastro.kyoto-u.ac.jp
- 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
Re: V551 Sgr: drefinite superoutburst of a new SU UMa star!
Dear Colleagues,
I can see some signature of possible "early superhumps" in Monard's
September 21 data (the object was probably experiencing the early relatively
rapid fading stage). This is not surprizing, as a long-period system
RZ Leo (Psh = 0.078529 d: Ishioka et al. 2001, PASJ 53, 905) also showed
the presence of early superhumps, which are the signature of WZ Sge-type
dwarf novae (cf. Kato 2002, PASJ 54, L11). The true identification
will be made when the exact superhump period is identified.
Regards,
Taichi Kato
VSNET Collaboration team
Return to Home Page
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
Powered by ooruri technology