RADIO-CONTINUUM OBSERVATIONS OF PLANETARY-NEBULA CANDIDATES FROM THE NORTHERN-HEMISPHERE

We analyzed radio continuum observations of unidentified IRAS point so urces with far IR colors that are typical of planetary nebulae. These IRAS-selected planetary nebula candidates are located outside the gala ctic bulge and were observed with the Westerbork Radio Synthesis Teles cope, We have detected 20 new planetary nebulae out of 82 observed can didates. The detected sources are very close to the galactic plane. Th e detection rate is highest in that part of the color-color diagram, w here planetary nebulae are expected to spend most time during their ev olution. The radio and IR properties are compared with PN detected in the same way in the galactic bulge and with optical planetary nebulae which fulfill the same selection criteria On average, the IR excess of the IRAS-selected and radio detected planetary nebula candidates is h igher than for the optical planetary nebulae.