Thiols in the Interstellar Medium: First Detection of HC(O)SH and Confirmation of C<sub>2</sub>H<sub>5</sub>SH
Lucas F. Rodríguez-Almeida, Izaskun Jiménez-Serra, Víctor M. Rivilla, Jesús Martín-Pintado, Shaoshan Zeng, Belén Tercero, Pablo de Vicente, Laura Colzi, Fernando Rico-Villas, Sergio Martín, Miguel A. Requena-Torres
Abstract
Abstract The chemical compounds carrying the thiol group (-SH) have been considered essential in recent prebiotic studies regarding the polymerization of amino acids. We have searched for this kind of compound toward the Galactic Center quiescent cloud G+0.693–0.027. We report the first detection in the interstellar space of the trans-isomer of monothioformic acid (t-HC(O)SH) with an abundance of ∼1 × 10 −10 . Additionally, we provide a solid confirmation of the gauche isomer of ethyl mercaptan (g-C 2 H 5 SH) with an abundance of ∼3 × 10 −10 , and we also detect methyl mercaptan (CH 3 SH) with an abundance of ∼5 × 10 −9 . Abundance ratios were calculated for the three SH-bearing species and their OH analogs, revealing similar trends between alcohols and thiols with increasing complexity. Possible chemical routes for the interstellar synthesis of t-HC(O)SH, CH 3 SH, and C 2 H 5 SH are discussed, as well as the relevance of these compounds in the synthesis of prebiotic proteins in the primitive Earth.