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[vsnet-chat 6277] V854 Oph is probably not a Mira star



   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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