  We observed five central stars of planetary nebulae (CSPN) in the Large
Magellanic Cloud (LMC) and three in the Small Magellanic Cloud (SMC) with the
Far Ultraviolet Spectroscopic Explorer (FUSE), in the range 905-1187 Ang. We
performed a model-based analysis of these spectra in conjunction with Hubble
Space Telescope (HST) spectra in the UV and optical range to determine stellar
and nebular parameters. The signature of hot (T >~ 2000 K) circumstellar
molecular hydrogen is found in the FUSE spectra of most objects. We also find
evidence of X-rays in the wind of LMC-SMP 76.
