([L72] LH 85-10)

Searching for LBV candidates in OB associations in the LMC, the object number 10, within the association LH 85, was found to be a luminous emission-line star. Due to the similarity of its blue spectrum with other B[e]SGs, it has been suggested as a new member of that group [96]. To date, no information about the presence of [O I] emission from that object is available. Moreover, its spectral energy distribution does not display the characteristic near-IR excess emission of B[e]SGs questioning the validity of this classification [108]. The star's position in the near-IR diagram coincides with the region populated by LBVs, supporting the erroneous classification. No WISE photometry is available for this object.
