Rotation-inversion transition of interstellar ammonia

Details Rotation-inversion transition of interstellar ammonia Rotation-inversion transition of interstellar ammonia

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...149..305z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 149, no. 2, Aug. 1985, p. 305-308.

Astronomy and Astrophysics

Astrophysics

2

Ammonia, Interstellar Gas, Molecular Clouds, Molecular Excitation, Astronomical Models, Inversions, Line Spectra, Molecular Oscillations, Optical Thickness

Scientific paper

A simplified model of the vibrational excitation of interstellar ammonia is examined. Assume that the rotation-inversion lines (e.g. JK = 10→00) and the inversion lines (e.g. JK = 11) are excited in the same radiation field with the radiation temperature Trd and the filling factor f. Using the observation data of the inversion lines (e.g. JK = 11) to select the suitable parameters, the rotation temperature, optical depth and the intensity of the rotation-inversion lines (e.g. JK = 10→00) can be estimated.

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