SEDs of star #22 (this work) and of the cLBV MN112 discovered by Gvaramadze et al. (2010). Flux densities in the DENIS, 2MASS, MSX, GLIMPSE, and WISE bands are plotted with diamonds, triangles, squares, crosses, and asterisks, respectively. The WISE 3 (11 μm) and 4 (20 μm) measurements were marked as affected by confusion. The long-dashed curves are black-bodies with the stellar effective temperatures. The dotted curves are modified black-bodies, which we created by adding to the continuum a 10–15% of free-free emission (∝ λ^-0.6), a warm dust component at 650 k, and a cold dust component at 150 k.