CS band intensity and column densities and production rates of 15 comets

Details CS band intensity and column densities and production rates of 15 comets CS band intensity and column densities and production rates of 15 comets

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....106.1237s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 106, no. 3, p. 1237-1240.

Astronomy and Astrophysics

Astronomy

1

Carbon Compounds, Comets, Interstellar Chemistry, Sulfides, Astronomical Spectroscopy, Emission Spectra, Franck-Condon Principle, Molecular Excitation, Photodissociation, Spectral Bands

Scientific paper

An accurate fluorescence efficiency of the CS(0,0) band and the lifetime of CS have been calculated at 1 AU heliocentric distance. Model-independent CS column densities and production rates are determined from derived fluorescent emission rates (g-factors) and lifetimes for 15 comets: Austin (1982g), Borrelly (1980i), Bradfield (1979X), Crommelin (1983n), Encke (1980), Encke (1984), Giacobini-Zinner (1984e), Halley (1982i), IRAS-Araki-Alcock (1983d), Meier (1980q), Panther (1980u), Stephan-Oterma (1980g), Tuttle (1980h), West (1975n), and Wilson (1986l).

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