The reaction between Si(+) and H2O - Interstellar implications

Details The reaction between Si(+) and H2O - Interstellar implications The reaction between Si(+) and H2O - Interstellar implications

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242..674w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Feb. 15, 1990, p. 674-677. Research supported by N

Astronomy and Astrophysics

Astronomy

6

Interstellar Chemistry, Molecular Clouds, Molecular Interactions, Silicon, Water, Energy Distribution, Ionic Collisions, Reaction Kinetics

Scientific paper

Based on room temperature experiments and theoretical considerations, it
has been determined that the reaction Si(+) + H2O yields SiOH(+) + H is
rapid at temperatures down to 10 K. The low abundance of SiO in cool
interstellar clouds such as TMC-1 is not a consequence of the slowness
of this reaction.

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