First detection of triply-deuterated methanol
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 13CH3OH, used to derive the column density of the main isotopomer CH3OH. The derived fractionation ratio [CD3OH]/[CH3OH] averaged on a 10'' beam is 1.4%. Together with previous CH2DOH and CHD2OH observations, the present CD3OH 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 H3+.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- March 2004
- DOI:
- 10.1051/0004-6361:20034490
- arXiv:
- arXiv:astro-ph/0311038
- Bibcode:
- 2004A&A...416..159P
- Keywords:
-
- ISM: abundances;
- ISM: molecules;
- stars: formation;
- ISM: individual: IRAS 16293-2422;
- Astrophysics
- E-Print:
- Accepted by A&