The rotational transitions of the interstellar molecule H2D(+)

Details The rotational transitions of the interstellar molecule H2D(+) The rotational transitions of the interstellar molecule H2D(+)

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..520k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, May-June 1987, p. 520-526. In Russian.

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Deuterium, Hydrogen, Interstellar Matter, Molecular Clouds, Molecular Rotation, Transition Probabilities, Astronomical Spectroscopy, Computational Astrophysics, Ion Production Rates, Radio Astronomy

Scientific paper

The line strengths and the A-coefficients for the rotational transitions of the para-H2D+ and ortho-H2D+ molecules are calculated. A possibility of the radio astronomical observations of H2D+ in the λ = 0.85 mm line is discussed. A method, based on H2D+ observations, for estimations of the gas ionization degree in dense interstellar clouds is suggested.

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