Detection of 2.6-millimeter radiation probably due to nitrogen sulfide

Details Detection of 2.6-millimeter radiation probably due to nitrogen sulfide Detection of 2.6-millimeter radiation probably due to nitrogen sulfide

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...200l.151k&link_type=abstract

Astrophysical Journal, vol. 200, Sept. 15, 1975, pt. 2, p. L151-L153

Astronomy and Astrophysics

Astronomy

8

Interstellar Matter, Millimeter Waves, Nitrogen Compounds, Radio Astronomy, Sulfides, Brightness Temperature, Electron Transitions, Molecular Energy Levels, Molecular Spectra, Radial Velocity, Radiation Measurement

Scientific paper

Results are reported for observations of millimeter-wavelength radiation in Sgr B2 at two frequencies corresponding to the transitions between the J = 5/2 and J = 3/2 Lambda-doublet sublevels in the 2 Pi(1/2) state of nitrogen sulfide. Difficulties in making a positive identification of the source of this radiation are discussed which result from the apparently anomalous ratio of the hyperfine components. However, it is noted that observations of the d-state by Gottlieb et al. (1975) showing the hyperfine components more exactly in their optically thin ratio confirm that the observed radiation is due to nitrogen sulfide.

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