We observed seven central stars of planetary nebulae ( CSPN ) in the Large Magellanic Cloud ( LMC ) with the Far Ultraviolet Spectroscopic Explorer ( FUSE ) , and performed a model-based analysis of these spectra in conjunction with Hubble Space Telescope ( HST ) spectra in the UV and optical range to determine the stellar and nebular parameters .
Most of the objects show wind features , and they have effective temperatures ranging from 38 to 60 kK with mass-loss rates of \simeq 5 \mbox { $ x 10 ^ { -8 } $ } { M _ { \odot } \ > yr ^ { -1 } } .
Five of the objects have typical LMC abundances .
One object ( SMP LMC 61 ) is a [ WC4 ] star , and we fit its spectra with He/C/O-rich abundances typical of the [ WC ] class , and find its atmosphere to be iron-deficient .
Most objects have very hot ( T \gtrsim 2000 K ) molecular hydrogen ( H _ { 2 } ) in their nebulae , which may indicate a shocked environment .
One of these ( SMP LMC 62 ) also displays O vi 1032-38 nebular emission lines , rarely observed in PN .