Microwave detection of interstellar cyanamide

Details Microwave detection of interstellar cyanamide Microwave detection of interstellar cyanamide

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201l.149t&link_type=abstract

Astrophysical Journal, vol. 201, Nov. 1, 1975, pt. 2, p. L149-L152.

Astronomy and Astrophysics

Astrophysics

29

Cyanamides, Emission Spectra, Interstellar Matter, Microwave Emission, Abundance, Astronomical Spectroscopy, Line Spectra, Molecular Spectra

Scientific paper

We report the detection of interstellar cyanamide (NH2CN) based on the observation of line emission in Sgr B2 at 80504.5 and 100629.5 MHz corresponding to the transitions 4(13)-3(12) and 5(14)-3(13). Statistical equilibrium calculations indicate a low column density (about 100 trillions per sq cm) arising from a rather high density region (greater than about 100,000 per cu cm).

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