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Thiols in the ISM: first detection of HC(O)SH and confirmation of C2H5SH.
Rodríguez-Almeida, Lucas F; Jimenéz-Serra, Izaskun; Rivilla, Víctor M; Martín-Pintado, Jesús; Zeng, Shaoshan; Tercero, Belén; de Vicente, Pablo; Colzi, Laura; Rico-Villas, Fernando; Martín, Sergio; Requena-Torres, Miguel A.
Afiliação
  • Rodríguez-Almeida LF; Centro de Astrobiolog'a (CSIC-INTA), Ctra Ajalvir km 4, 28850, Torrejon de Ardoz, Madrid, Spain.
  • Jimenéz-Serra I; Centro de Astrobiolog'a (CSIC-INTA), Ctra Ajalvir km 4, 28850, Torrejon de Ardoz, Madrid, Spain.
  • Rivilla VM; Centro de Astrobiolog'a (CSIC-INTA), Ctra Ajalvir km 4, 28850, Torrejon de Ardoz, Madrid, Spain.
  • Martín-Pintado J; INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125, Florence, Italy.
  • Zeng S; Centro de Astrobiolog'a (CSIC-INTA), Ctra Ajalvir km 4, 28850, Torrejon de Ardoz, Madrid, Spain.
  • Tercero B; Star and Planet Formation Laboratory, Cluster for Pioneering Research, RIKEN,2-1 Hirosawa, Wako, Saitama, 351-0198, Japan.
  • de Vicente P; Observatorio de Yebes (IGN), Cerro de la Palera s/n, 19141, Guadalajara, Spain.
  • Colzi L; Observatorio de Yebes (IGN), Cerro de la Palera s/n, 19141, Guadalajara, Spain.
  • Rico-Villas F; Centro de Astrobiolog'a (CSIC-INTA), Ctra Ajalvir km 4, 28850, Torrejon de Ardoz, Madrid, Spain.
  • Martín S; INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125, Florence, Italy.
  • Requena-Torres MA; Centro de Astrobiolog'a (CSIC-INTA), Ctra Ajalvir km 4, 28850, Torrejon de Ardoz, Madrid, Spain.
Astrophys J Lett ; 912(1)2021 May 01.
Article em En | MEDLINE | ID: mdl-34257894
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 ~ 1 × 10-10. Additionally, we provide a solid confirmation of the gauche isomer of ethyl mercaptan (g-C2H5SH) with an abundance of ~ 3 × 10-10, and we also detect methyl mercaptan (CH3SH) with an abundance of ~ 5 × 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, CH3SH and C2H5SH are discussed, as well as the relevance of these compounds in the synthesis of prebiotic proteins in the primitive Earth.
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Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Diagnostic_studies Idioma: En Revista: Astrophys J Lett Ano de publicação: 2021 Tipo de documento: Article País de afiliação: Espanha

Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Diagnostic_studies Idioma: En Revista: Astrophys J Lett Ano de publicação: 2021 Tipo de documento: Article País de afiliação: Espanha