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[vsnet-gcvs 356] V2101 Oph is a Mira star

Date: Sun, 4 May 2003 19:45:15 +0900 (JST)
To: vsnet-gcvs@ooruri.kusastro.kyoto-u.ac.jp
From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
Subject: [vsnet-gcvs 356] V2101 Oph is a Mira star
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   According to ASAS-3 survey, V2101 Oph (previously suggested
to be a dwarf nova, later confirmed to be a late-type star)
is definitely a Mira star.  The period is 680/N (N=2 or 3) d.
(V max about 12.4).

Regards,
Taichi Kato

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