Possible new interstellar masers

Details Possible new interstellar masers Possible new interstellar masers

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980rspsa.373..269g&link_type=abstract

Royal Society (London), Proceedings, Series A - Mathematical and Physical Sciences, vol. 373, no. 1753, Nov. 25, 1980, p. 269-28

Mathematics

4

Diatomic Molecules, Interstellar Masers, Molecular Collisions, Population Inversion, Matrices (Mathematics), Molecular Energy Levels, Molecular Ions, Molecular Rotation

Scientific paper

A collisional mechanism for the production of population inversion in
the lambda-doublet sublevels of the lowest rotational energy levels of
diatomic molecules is considered. This leads to the conclusion that not
only should the known celestial masers, OH and CH, be capable of
exhibiting stimulated emission, but also HF(+), HCl(+) and SH

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