LiH molecules in dense interstellar clouds

Details LiH molecules in dense interstellar clouds LiH molecules in dense interstellar clouds

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...36v&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Jan.-Feb. 1986, p. 36-42. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Interstellar Gas, Lithium Hydrides, Molecular Clouds, Chemical Reactions, Infrared Astronomy, Line Spectra, Molecular Rotation

Scientific paper

The abundances of LiH molecules in interstellar clouds are estimated.
Calculations are then made of the excitation temperatures of various LiH
rotational levels and of expected radiation fluxes in IR lines
corresponding to LiH rotational transitions. The possibility of
observing these lines is discussed.

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