Here we present the results of 1.3 millimetre continuum measurements f
or intermediate-mass stars in the Chamaeleon system of dark clouds. Th
e detected millimetre radiation is most probably thermal emission from
cold circumstellar dust grains. The measured millimetre fluxes are co
mbined with infrared observations to model the broad-band spectral ene
rgy distribution (SED). In this way the parameters of the emission reg
ions are determined.