An analysis of the spectrophotometric and photometric observations of comets 1967II, 1968I, 1968V, and 1968VI

Details An analysis of the spectrophotometric and photometric observations of comets 1967II, 1968I, 1968V, and 1968VI An analysis of the spectrophotometric and photometric observations of comets 1967II, 1968I, 1968V, and 1968VI

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991em%26p...53..205d&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 53, June 1991, p. 205-216.

Computer Science

Numerical Analysis

3

Astronomical Photometry, Comets, Particle Emission, Spectrophotometry, Carbon, Cyanogen, Formalism, Numerical Analysis

Scientific paper

Emission fluxes of CN, C2, and C3 carbon-bearing molecular species observed in the coma of comets Rudnicki (1967II), Ikeya-Seki (1968I), Whitaker-Thomas (1968V), and Honda (1968VI) are analyzed in the framework of Haser's (1957) 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. It is shown that comets Ikeya-Seki (1968I) and Honda (1968VI) have the same mean color indices (B-V) and (U-B).

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