We report ROSAT Position Sensitive Proportional Counter (PSPC) observa
tions of four planetary nebulae. The observations show that all four n
ebulae have two-component spectra. A two-component model consisting of
a blackbody and a Raymond-Smith thermal plasma is fitted to the obser
ved ROSAT PSPC spectra of NGC 1535, Abell 36, and NGC 7293. For all th
ree cases, the temperatures of the blackbody component are apparently
higher than those of the stellar photospheres, indicating nonblackbody
atmospheres. In all cases, the temperatures of the high-energy compon
ent can be attributed to a hot plasma associated with the possible ste
llar coronae or the ''hot bubbles'' predicted by the interacting winds
model. The spectral energy distribution of NGC 1535 is constructed an
d modeled by incorporating our X-ray spectrum into existing data in UV
, optical, near-infrared, and far-infrared wavelengths.