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AA Dor is an eclipsing, close, post common-envelope binary (PCEB). We presenta detailed spectral analysis of its sdOB primary star based on observationsobtained with the Far Ultraviolet Spectroscopic Explorer (FUSE). Due to astrong contamination by interstellar absorption, we had to model both, thestellar spectrum as well as the interstellar line absorption in order toreproduce the FUV observation well and to determine the photospheric parametersprecisely.

FUV Spectroscopy of the sdOB Primary of the Eclipsing Binary System AA Dor