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Issue A&A
Volume 416, Number 1, March II 2004
Page(s) 159 - 163
Section Interstellar and circumstellar matter
DOI http://dx.doi.org/10.1051/0004-6361:20034490



A&A 416, 159-163 (2004)
DOI: 10.1051/0004-6361:20034490

First detection of triply-deuterated methanol

B. Parise1, A. Castets2, E. Herbst3, E. Caux1, C. Ceccarelli4, I. Mukhopadhyay5 and A. G. G. M. Tielens6

1  CESR CNRS-UPS, BP 4346, 31028 Toulouse Cedex 04, France
2  Observatoire de Bordeaux, BP 89, 33270 Floirac, France
3  Department of Physics, The Ohio State University, 174 W. 18th Ave. Columbus, OH 43210-1106, USA
4  Laboratoire d'Astrophysique, Observatoire de Grenoble, BP 53, 38041 Grenoble Cedex 09, France
5  Dakota State University, 820 N. Washington Ave., Madison, SD 57042, USA
6  SRON, PO Box 800, 9700 AV Groningen, The Netherlands

(Received 7 August 2003 / Accepted 3 November 2003)

Abstract
We report the first detection of triply-deuterated methanol, with 12 observed transitions, towards the low-mass protostar IRAS 16293-2422, as well as multifrequency observations of 13CH 3OH, used to derive the column density of the main isotopomer CH 3OH. The derived fractionation ratio [ CD 3OH] /[ CH 3OH] averaged on a 10 '' beam is 1.4%. Together with previous CH 2DOH and CHD 2OH observations, the present CD 3OH observations are consistent with a formation of methanol on grain surfaces, if the atomic D/H ratio is 0.1 to 0.3 in the accreting gas. Such a high atomic ratio can be reached in the framework of gas-phase chemical models including all deuterated isotopomers of H 3+.


Key words: ISM: abundances -- ISM: molecules -- stars: formation -- ISM: individual: IRAS 16293-2422

Offprint request: B. Parise, Berengere.Parise@cesr.fr

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