The classification spectra were obtained using the IDS spectrograph of
the Isaac Newton Telescope, La Palma on the night of 1998 August 2.
The R1200B grating was employed with a slit width of 1.15 arcsec and the
EEV12 CCD. This gives a dispersion of Å/pixel.
A central wavelength was chosen of 4300 Å, giving a
a wavelength range of 3670 - 5070 Å. Measurements of
interstellar features in the spectra give a full width half maximum
corresponding to a velocity resolution of
km s-1.
In addition to our
Be star sample we obtained spectra of
30 MK standards in the range O9 to B9.5, mainly of luminosity classes
III and V (Table 3).
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