Comet Halley was observed with a high-resolution Fabry-Perot spectrometer (X78X. ~4 X 10 4 ) in the wavelengths [O i] and NH 2 (0-8-0) in the neighborhood of 6300 Â during 1986 April 13-15. The [O i] line and NH 2 rotational lines were spectrally well separated by the interferometer. The profile analysis shows the profiles of [O i] and NH 2 to be symmetric with the linewidths ~ 3.5-3 km s' 1 . The ratio (NH 2 Á.6298.6 (2 12 -2 02 ))/[O i] is ~ 0.5. Observations were also attempted in Ha, but no clear signal was detectable above the noise within the field of view (50") of the instrument. Upper limits consistent with other results are derived for Ha. This paper discusses the observations briefly followed by details of the analysis and the results.