A potential extraterrestrial species - The SH(+) molecular ion

Details A potential extraterrestrial species - The SH(+) molecular ion A potential extraterrestrial species - The SH(+) molecular ion

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...142..346h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 142, no. 2, Jan. 1985, p. 346-350.

Astronomy and Astrophysics

Astrophysics

11

Cometary Atmospheres, Hydrogen Sulfide, Interstellar Matter, Molecular Ions, Molecular Spectra, Oscillator Strengths, Infrared Spectra, Radiative Lifetime, Transition Probabilities, Visible Spectrum, Wavelengths

Scientific paper

Relevant spectroscopic properties in the UV, IR, and MW regions are collected in order to aid detection of the SH(+) molecular ion in astrophysical objects. The ion is likely to be present in shock-heated regions of the interstellar medium and in cometary atmospheres. Sets of rotational term values, wavelengths, and Franck-Condon factors are given, and the corresponding transition probabilities, oscillator strengths, and equivalent widths are estimated. The data presented are expected to facilitate observation of the IR spectrum in the laboratory by laser techniques, which, in turn, may assist in detection of SH(+) in the millimeter and submillimeter regions both in the laboratory and in the interstellar medium.

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