Spectrophotometric study of periodic Comet Halley (1982i)

Details Spectrophotometric study of periodic Comet Halley (1982i) Spectrophotometric study of periodic Comet Halley (1982i)

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989em%26p...45...17g&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 45, April 1989, p. 17-27.

Computer Science

1

Chemical Composition, Emission Spectra, Halley'S Comet, Spectrophotometry, Visible Spectrum, Carbon Compounds, Cyanogen, Methyl Compounds, Nitrogen Hydrides

Scientific paper

Spectral scans of the head of periodic Comet Halley (1982i) have been presented and analyzed in detail in the optical region 3200-7000 A for ten nights during the preperihelion period. Emission features due to NH, CN, CH, C3, and C2 molecules have been identified. The behavior of the variation of different emission lines strength as a function of heliocentric distance has been investigated. It is found that the comet exhibits night-to-night variation of brightness. The abundances and production rates of CN and C2 species have also been derived.

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