Detection of HCN in comet P/Halley

Astronomy and Astrophysics – Astronomy

Scientific paper

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Cometary Atmospheres, Halley'S Comet, Hydrocyanic Acid, Millimeter Waves, Radio Astronomy, Beam Switching, Radial Velocity, Spectral Line Width, Thermodynamic Equilibrium, Comets, Halley, Hydrogen Cyanide, Compostion, Comae, Telescope Methods, Earth-Based Observations, Production Rate, Intensity, Radio Methods, Spectra, Spectrometry, Parameters, Data, Jetting, Analysis, Molecules

Scientific paper

An account is given of the millimeter observations of comet Halley at the Onsala Space Observatory during November and December 1985. The J = 1-0 line of HCN at 88.63 GHz was detected in the comet's coma during the period Nov. 8-29, 1985, using the 20-m millimeter wave telescope. The line intensity varied by a factor of 2.2 or more during the observing period. The lines detected were of the F = 2-1 and F = 1-1 hyperfine transitions. On November 9, 10 and again on November 12, 13, weak evidence was seen for a velocity shift in both the main line and the F = 1-1 satellite line. The lines were redshifted by 0.9 km/s relative to the velocity of the comet and were narrower (0./4 km/s) than other detected lines. This may point to anisotropic gas ejection from the comet.

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