0 citations
Interstellar methyl mercaptan
The Astrophysical Journal1979Vol. 234, pp. L139–L139
Citations Over Time
Abstract
Methyl mercaptan (CH3SH) has been identified in Sgr B2 from observations of six lines in its millimeter-wave spectrum. The CH3SH rotational temperature and column density in Sgr B2 are T(rot) = 9 plus or minus 3 K and N = 1.5 plus or minus 0.2 x 10 to the 14th per sq cm, respectively. The CH3SH/CH3OH ratio is apparently not greatly different from the cosmic S/O ratio.
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
- → Organometallic Chemistry in the interstellar medium(2002)4 cited
- → A piece of interstellar medium in the laboratory: the PIRENEA experiment(2002)18 cited