(J013242.26+302114.1)

The optical spectra of this object display all typical B[e]SG characteristics, but the star's IR colors displace it clearly from the sample of confirmed B[e]SGs. It has excess emission at 8 μm due to PAHs [99]. The JHK magnitudes sugges<sup>t</sup> that J013242.26+302114.1 falls into the region of late-type stars and stars with a late-type companion, respectively, [20,144]. This classification is supported by the WISE colors, although regular late-type stars typically have slightly negative W1–W2 colors. Considering only the WISE photometry, J013242.26+302114.1 would fit to the region populated by LBVs. This objects clearly needs to be investigated in more detail for a proper classification.
