  We present infrared (0.97-2.45 micron) spectra of the intermediate polars PQ
Gem (RE0751+14), BG CMi and EX Hya. The spectra show strong Paschen, Brackett
and HeI emission lines from the accretion disc/stream. The infrared continua of
PQ Gem and BG CMi can be represented by blackbodies of temperatures 4500 K and
5100 K, respectively, or by power-laws of the form f_nu \propto nu^(0.6,0.9),
respectively, and show no evidence of secondary star features. The continuum of
EX Hya is doiminated by water bands from the red-dwarf secondary star, which
has a spectral type of ~M3. Despite showing circular polarization, PQ Gem and
BG CMi show no evidence for cyclotron humps and hence we are unable to measure
their magnetic field strengths; any cyclotron emission present must contribute
less than ~3 per cent of the infrared continuum flux.
