Spectrophotometric study of P/Halley during POST perihelion passage

Details Spectrophotometric study of P/Halley during POST perihelion passage Spectrophotometric study of P/Halley during POST perihelion passage

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991em%26p...54...13g&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 54, July 1991, p. 13-17.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Carbon, Cyanogen, Halley'S Comet, Spectral Emission, Chemical Composition, Emission Spectra, Spectral Bands, Vibrational Spectra, Visible Spectrum

Scientific paper

Spectrophotometric observations of P/Halley are presented for four nights in the optical region (3200-7000 A) during post-perihelion period. Emission features due to CN, CH, C3, and C2 molecules are identified and the total apparent fluxes in each emission band are measured. It is found that the comet displays large variations in the emission bands as well as continuum.

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