  We have searched for evidence of emission at 15 microns with ISOCAM and at 90
microns with ISOPHOT from dust orbiting six nearby pulsars, both in binaries
and in isolation, located at distances between about 100 to 1000 pc. No
emission was detected at any of the pulsar positions, and for the nearest
pulsar J0108-1431 the 3 sigma upper limits on the flux density is about 66 mJy
at 15 microns and 22.5 mJy at 90 microns. Upper limits on the masses of
circumpulsar dust are inferred at a given temperature using a simple modelling
of the radiated flux; they are compared to upper limits of orbiting mass
obtained with the dust heating model of Foster & Fisher (1996). These results
suggest that it is unlikely that any of them have sufficiently massive,
circumpulsar discs out of which planets may form in the future.
