  We present H band (1.53 - 1.69 micron) spectra of 57 isolated Be stars of
spectral types O9-B9 and luminosity classes III,IV & V. The HI Brackett (n-4)
series is seen in emission from Br 11-18, and FeII emission is also apparent
for a subset of those stars with HI emission. No emission from species with a
higher excitation temperature, such as He II or CIII is seen, and no forbidden
line emission is present. A subset of 12 stars show no evidence for emission
from any species; these stars appear indistinguishable from normal B stars of a
comparable spectral type. In general the line ratios constructed from the
transitions in the range Br 11-18 do not fit case B recombination theory
particularly well. Strong correlations between the line ratios with Br-gamma
and spectral type are found. These results most likely represent systematic
variations in the temperature and ionization of the circumstellar disc with
spectral type. Weak correlations between the line widths and projected
rotational velocity of the stars are observed; however no systematic trend for
increasing line width through the Brackett series is observed.
