  Inspired by an appeal to the community from Walborn (these proceedings) we
decided to solve the long-standing problem concerning the nature of the
4486,4504A emission lines, which are frequently observed in O-type spectra and
which are particularly prominent in supergiants. We claim that these lines
emerge from sulfur, namely by de-excitation of a highly excited S IV doublet
state. We prove this by an exploratory NLTE calculation with a detailed model
atom.
