THZ SPECTROSCOPY OF ACETALDEHYDE AND SEARCH OF $^{13}$C SPECIES IN ORION

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2012

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Ohio State University

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Acetaldehyde (CH$_3$CHO) is one of the high priority complex organic molecules for the astrophysical community. There is a lack of data concerning the $^{13}$C species since the measurements are limited to 40 GHz~{\bf26}, (1957) 1695} up to date. This molecule displays a large amplitude motion: the hindered rotation of the methyl group with respect to the rest of the molecule. The analysis is performed with RAM36 code~{\bf259}, (2010) 26} which used the Rho Axis Method. Last year we presented the analysis of the millimeterwave spectra of the $^{13}$CH$_3$CHO species, {\em 66th International Symposium on Molecular Spectroscopy (2011)}}. We extended the analysis to the THz range of the vibrational ground state for both species. We are also analyzing the first torsional state ($\approx$140 cm$^{-1}$) for two reasons: first, this permits to remove correlation between parameters. Second, this state contribute to the partition function even at ISM temperature (100--150~K) since there is an influence on the column density determined in case of detection. The searches of these isotopomers are in progress in ORION.

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This work was supported by the CNES and the Action sur Projets de l'INSU, PCMI. This work was also done under the ANR-08-BLAN-0054.
Author Institution: Laboratoire PhLAM, CNRS UMR 8523, Universite; Institute of Radio Astronomy of NASU, Chervonopraporna Str., 4, 61002 Kharkov, Ukraine; Centro de Astrobiologia (CSIC-INTA). Laboratory of Molecular Astrophysics.; Department of Astrophysics.; Ctra de Ajalvir,Km 4, 28850 Torrejon de Ardoz, Madrid, Spain; Sciences Chimiques de Rennes, UMR 6226 CNRS-ENSCR, Avenue du General Leclerc, CS 50837, 35708 Rennes Cedex 7, France.

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