tgandet on 18-Mar-2011 00:31:06 GMT about * 18 And
Cote and van
Kerkwijk (1993, A&A, 274, 870)
discovered this star to be a Be star, with emission in H-alpha well below the continuum.
Granada et. al. (2010, AJ, 139, 1983)
state the spectral type is B9Ve and describe it as a weak shell line star, with weak emission at H-alpha.
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View annotation on * 18 And object