emamajek on 25-Apr-2010 23:27:43 GMT about V* V1215 Cen
This star is listed as a possible member ("Y?") of the TW Hydra Association in Mamajek (2005; http://adsabs.harvard.edu/abs/2005ApJ...634.1385M ). This assessment has not changed - it is likely to be either a member of the TW Hydra Association or the Lower Centaurus-Crux subgroup of Sco-Cen. For either kinematic solution, its proper motion is consistent with a cluster parallax distance of ~80 +- 5 pc (unusually distant for a TWA members, but unusually close for a LCC members).
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View annotation on V* V1215 Cen object