Predictions on finding the SiH/+/ and SiH in interstellar space

Details Predictions on finding the SiH/+/ and SiH in interstellar space Predictions on finding the SiH/+/ and SiH in interstellar space

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..56..415d&link_type=abstract

Astrophysics and Space Science, vol. 56, no. 2, July 1978, p. 415-419.

Astronomy and Astrophysics

Astronomy

3

Interstellar Chemistry, Molecular Ions, Radio Astronomy, Silicon Compounds, Interstellar Matter, Molecular Rotation, Radicals, Vibrational Spectra

Scientific paper

Frequencies are computed for transitions in the SiH(+) and SiH molecules which are expected to occur in the millimeter region usually covered by radio astronomy. These molecules are expected to be in low-temperature sources whose kinetic temperatures are not greater than about 20 K. On the basis of binary gas-phase reactions, the formation and destruction of the SiH(+) and the SiH radicals are also discussed.

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