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. Tielens61 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
SIMBAD Objects
© ESO 2004

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