Spectral characteristics of the interstellar molecule H3O(+)

Details Spectral characteristics of the interstellar molecule H3O(+) Spectral characteristics of the interstellar molecule H3O(+)

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..325k&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Oct. 1987, p. 325-334. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Interstellar Gas, Molecular Clouds, Positive Ions, Spectral Energy Distribution, Hydrogen Compounds, Line Spectra, Molecular Ions, Molecular Rotation, Optical Thickness

Scientific paper

The line strengths and the probabilities of inversion-rotational
transitions of the hydroxonium ion H3O+ are
calculated. Excpected optical thicknesses of typical interstellar clouds
are estimated for H3O+ lines of radio astronomical
interest (λ = 0.8 - 1.0 mm).

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