Photochemical studies of S2 formation and their implications on the source and evolution of comets.

Details Photochemical studies of S2 formation and their implications on the source and evolution of comets. Photochemical studies of S2 formation and their implications on the source and evolution of comets.

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.249..143g&link_type=abstract

ESA Spec. Publ., ESA SP-249, p. 143 - 151

Computer Science

2

Comet 1983 Vii Iras-Araki-Alcock, Comets:Evolution, Comets:Interstellar Matter, Comets:Sulfur, Interstellar Matter:Comets

Scientific paper

The formation of S2 by ultraviolet photoprocessing of interstellar ices is shown to be a plausible explanation for the observation of this molecule in comet IRAS-Araki-Alcock 1983d. Not only S2 is to be expected in cometary ices but also such products as SH, SO, CS, CS2, HSO, OCS etc. The composition of the processed interstellar analog ices is compared with molecular production rates in comets.

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