Study of the A-X (0,0) band profile of CS in comets

Details Study of the A-X (0,0) band profile of CS in comets Study of the A-X (0,0) band profile of CS in comets

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...271..326k&link_type=abstract

Astronomy and Astrophysics, Vol. 271, p. 326 (1993)

Astronomy and Astrophysics

Astrophysics

2

Comets, Cs Molecule, Molecular Processes, Rotational Population

Scientific paper

The synthetic rotational profile of the A-X (0,0) band of CS have been compared with the observed profile for comets Bradfield (1979 X), P/Giacobini-Zinner and P/Halley. The synthetic profile for a gas temperature ˜200 K gives a reasonably good fit to the observed profile for comets Bradfield (1979 X) and P/Giacobini-Zinner. However for comet P/Halley there is some disagreement in a small wavelength region. Extensive time-dependent calculations of various types have been carried out to see whether freshly formed molecules could remove the observed discrepancy. This is also associated with serious difficulties.

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