0 citations
Interstellar isothiocyanic acid
The Astrophysical Journal1979Vol. 234, pp. L143–L143
Citations Over TimeTop 14% of 1979 papers
Abstract
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.
Related Papers
- → Gas-phase Chemistry in the Interstellar Medium: The Role of Laboratory Astrochemistry(2022)41 cited
- → Cosmic-ray astrochemistry(2013)46 cited
- → Is the reaction between formic acid and protonated aminomethanol a possible source of glycine precursors in the interstellar medium?(2015)19 cited
- → A piece of interstellar medium in the laboratory: the PIRENEA experiment(2002)18 cited
- Laboratory for Geochemistry, Cosmochemistry and Astrochemistry marks thirty years of Scientific Research(2008)