Accurate spectroscopic characterization of ethyl mercaptan and dimethyl sulfide isotopologues: a route toward their astrophysical detection
Journal Article
·
· Astrophysical Journal
- Dipartimento di Chimica, "Giacomo Ciamician," Università diBologna, Via F. Selmi 2, I-40126 Bologna (Italy)
- Departamento de Química y Física Teóricas, Institsuto de Estructura de la Materia, IEM-C.S.I.C., Serrano 121, Madrid E-28006 (Spain)
- Doctora Vinculada IEM-CSIC, Departamento de Ingeniería Civil, Cátedra de Química, E.U.I.T. Obras Públicas, Universidad Politécnica de Madrid (Spain)
- Departamento de Física Aplicada, Facultad de Ciencias Experimentales, Unidad Asociada IEM-CSIC-U.Huelva, Universidad de Huelva, E-21071 Huelva (Spain)
- Université Paris-Est, Laboratoire de Modélisation et Simulation Multi Echelle, MSME UMR 8208 CNRS, 5 boulevard Descartes, F-77454 Marne-la-Vallée (France)
Using state-of-the-art computational methodologies, we predict a set of reliable rotational and torsional parameters for ethyl mercaptan and dimethyl sulfide monosubstituted isotopologues. This includes rotational, quartic, and sextic centrifugal-distortion constants, torsional levels, and torsional splittings. The accuracy of the present data was assessed from a comparison to the available experimental data. Generally, our computed parameters should help in the characterization and the identification of these organo-sulfur molecules in laboratory settings and in the interstellar medium.
- OSTI ID:
- 22369980
- Journal Information:
- Astrophysical Journal, Vol. 796, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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