We propose to observe bright massive B[e] supergiants in the LMC
 and SMC in order to study their circumstellar environment. This
 environment is very complex, with regions where gas flows out at
 high velocity and other regions where gas is very cool, dust
 is formed and the outflow velocities are low. It is suggested that
 B[e] stars are rapidly rotating post-main-sequence stars, but the
 precise nature of the stars (just evolved off the main sequence,
 or post-red-supergiant) is not understood. The ISO observations
 will provide us with new insights into the mass loss and wind
 structure by measuring the 2-12 micron spectrum in low resolution.
 This will give us the line strengths of H and He emission lines,
 as well as several forbidden lines. In addition, we request for
 the brightest three stars full SWS scans in order to investigate
 the 10-45 micron spectral region. Many dust and line features
 can be found that are crucial for a better understanding of the
 evolutionary status of these stars. ISO is the only instrument
 that will be able to provide the 10-45 micron data with a resolution
 of 500-1000, and the requested PHOT-S spectra are very difficult
 to obtain from the ground.