jgsimbad on 11-Oct-2012 11:00:44 GMT about
This star is most evidently not a Mira.
At best it can be described as GCVS variability type Lb (late spectral type irregular variable).
<http://www.astrouw.edu.pl/cgi-asas/asas_variable/231912+1711.6,asas3,0,0,1600,400>
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