{ "id": "2104.08036", "version": "v1", "published": "2021-04-16T11:14:16.000Z", "updated": "2021-04-16T11:14:16.000Z", "title": "Thiols in the ISM: first detection of HC(O)SH and confirmation of C$_2$H$_5$SH", "authors": [ "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" ], "comment": "16 pages, 6 figures, article accepted in Astrophysical Journal Letters", "categories": [ "astro-ph.GA" ], "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 compounds toward the Galactic Centre 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 $\\sim\\,$1$\\,\\times\\,$10$^{-10}$. Additionally, we provide a solid confirmation of the gauche isomer of ethyl mercaptan (g-C$_2$H$_5$SH) with an abundance of $\\sim\\,$3$\\,\\times\\,$10$^{-10}$, and we also detect methyl mercaptan (CH$_3$SH) with an abundance of $\\sim\\,$5$\\,\\times\\,$10$^{-9}$. Abundance ratios were calculated for the three SH-bearing species and their OH-analogues, revealing similar trends between alcohols and thiols with increasing complexity. Possible chemical routes for the interstellar synthesis of t-HC(O)SH, CH$_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.", "revisions": [ { "version": "v1", "updated": "2021-04-16T11:14:16.000Z" } ], "analyses": { "keywords": [ "first detection", "confirmation", "galactic centre quiescent cloud", "detect methyl mercaptan", "prebiotic studies" ], "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable" } } }