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[vsnet-chat 6277] V854 Oph is probably not a Mira star
- Date: Fri, 2 May 2003 17:36:47 +0900 (JST)
- To: vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp,vsnet-gcvs@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-chat 6277] V854 Oph is probably not a Mira star
- Delivered-To: vsnet-chat-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
According to the ASAS-3 data, V854 Oph (GCVS M: range
11-16p, identification studied by Yoshida-san in the past)
does not apparently show Mira-type variation. The past reported
variation may have been resulted from a different origin.
Regards,
Taichi Kato
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