A&A 416, 801-810 (2004)
DOI: 10.1051/0004-6361:20034602
Molecular complexes theoretical computations between methanol and carbon dioxide and their implications in the interstellar ice mantles
A. Klotz1, 2, T. Ward2 and E. Dartois31 Centre d'Étude Spatiale des Rayonnements, Observatoire Midi-Pyrénées (CNRS-UPS), BP 4346, 31028 Toulouse Cedex 04, France
2 Laboratoire de Physique Quantique, Institut de Recherche sur les Systèmes Atomiques et Moléculaires Complexes (UPS-CNRS), 118 Route de Narbonne, 31400 Toulouse, France
3 Institut d'Astrophysique Spatiale (CNRS), Orsay, France
(Received 21 May 2003 / Accepted 7 November 2003)
Abstract
Theoretical computations were carried out on the
molecular complex between methanol and carbon dioxide.
These calculations explain the broadening of the
15
m spectral feature observed in interstellar
ices. This feature is assigned to the bending of
C-O of the carbon dioxide and we confirm that
the broadening is compatible with methanol
interactions of the electron donor acceptor type.
Extra interactions are also investigated
and can be implied in the broadening.
Key words: molecular: spectroscopy infrared
Offprint request: A. Klotz, klotz@cesr.fr
© ESO 2004
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