ISOCAM OBSERVATIONS OF CYG X-3 - SEARCH FOR A HOT STELLAR WIND

Six CAM observations have been made in the 4 - 14 mu m wavelength regi on to search for further evidence of emission from a hot stellar wind. Initial results suggest that the spectrum detected by Fender et al. u sing UKIRT extends into the wavelength region covered by ISOCAM. There is also evidence that the source is variable on timescales of approxi mate to 70 seconds.