On the identification of CO in the visible spectrum of comet Bradfield 1980 T

Details On the identification of CO in the visible spectrum of comet Bradfield 1980 T On the identification of CO in the visible spectrum of comet Bradfield 1980 T

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ncgb.conf..131c&link_type=abstract

IN: Workshop on the Need for Coordinated Ground-Based Observations of Halley's Comet, Paris, France, April 29, 30, 1982, Proceed

Physics

2

Carbon Monoxide, Cometary Atmospheres, Visible Spectrum, Emission Spectra, Line Spectra, Spectrum Analysis

Scientific paper

CO emission lines between 4000 and 9000 A have been identified for the first time in the comet Bradfield 1980 t, by means of spectra obtained with the 122- and 182-cm Asiago Observatory telescopes, and the absolute fluxes of 15 lines have been determined by means of a Reticon detector. Preliminary theoretical calculations on possible parent molecules and production rates are presented. The emissions are most likely produced through the dissociative recombination of an ion, such as HCO(+).

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