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[vsnet-gcvs 332] 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-gcvs 332] V854 Oph is probably not a Mira star
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   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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