On the Detection of Dimethyl Sulfide in Space
M. Sanz-Novo, V. M. Rivilla, C. P. Endres, V. Lattanzi, I. Jiménez-Serra, L. Colzi, S. Zeng, A. Megías, Á. López-Gallifa, A. Martínez-Henares, D. San Andrés, B. Tercero, P. de Vicente, S. Martín, M. A. Requena-Torres, P. Caselli, and J. Martín-Pintado
reported on the
On the Abiotic Origin of Dimethyl Sulfide: Discovery of Dimethyl Sulfide in the Interstellar Medium
Astrophys. J. Lett. 980, Art. No. L37 (2025).
Dimethyl sulfide, (CH3)2S, was identified in the course of a molecular line survey of the Galactic center cold molecular cloud G+0.693−0.027 carried out with the Yebes 40 m and IRAM 30 m radio telescopes. Several b-type lines with 2 ≤ J ≤ 9, Ka ≤ 4, and with unresolved internal rotation splitting were assigned with reasonable signal-to-noise ratios, but a number of these are blended to different amounts. The excitation temperatures was determined as 13 ± 3 K. Its column density is about a factor of 30 lower than than of its oxigen homolog dimethyl ether and about a factor of 1.6 lower than its ethanethiol isomer.
Contributor(s): H. S. P. Müller; 02, 2025