Physics
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992em%26p...56...61d&link_type=abstract
Earth, Moon, and Planets (ISSN 0167-9295), vol. 56, no. 1, Jan. 1992, p. 61-74. Research supported by CNPq.
Physics
3
Carbon, Comets, Cyanogen, Fluorescence, Molecular Gases, Radicals
Scientific paper
Emission fluxes of CN, C2, and C3 carbon-bearing molecular species observed in the coma of Comets Bennett, West, P Halley, Hartley-Good and Bradfield are analyzed in the framework of the Haser model. CN, C2 and C3 production rates are determined using recently derived fluorescence efficiencies. The dependence of CN, C2, and C3 production rates on the heliocentric distance and the possible correlations among these radicals is studied and briefly discussed.
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