Interstellar isothiocyanic acid

Details Interstellar isothiocyanic acid Interstellar isothiocyanic acid

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234l.143f&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 234, Dec. 1, 1979, p. L143-L145.

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15

Astronomical Spectroscopy, Cyano Compounds, Interstellar Gas, Molecular Spectra, Sulfur Compounds, Abundance, Line Spectra, Millimeter Waves, Molecular Rotation

Scientific paper

Isothiocyanic acid (HNCS) has been identified in Sgr B2 from millimeter-wave spectral line observations. We have definitely detected three rotational lines, and have probably detected two others. The rotational temperature of HNCS in Sgr B2 is 14 plus or minus 5 K, its column density is 2.5 plus or minus 1.0 x 10 to the 13th per sq cm, and its abundance relative to HNCO is consistent with the cosmic S/O ratio, 1/42.

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