Deuterated methanol toward NGC 7538-IRS1
arXiv:1905.09798 · doi:10.1051/0004-6361/201834948
Abstract
We investigate the deuteration of methanol towards the high-mass star forming region NGC 7538-IRS1. We have carried out a multi-transition study of CHOH, CHOH and of the deuterated fllavors, CHDOH and CHOD, between 1.0--1.4 mm with the IRAM-30~m antenna. In total, 34 CHOH, 13 CHDOH lines and 20 CHOD lines spanning a wide range of upper-state energies (E) were detected. From the detected transitions, we estimate that the measured D/H does not exceed 1, with a measured CHDOH/CHOH and CHOD/CHOH of about (328)10 and (104)10, respectively. This finding is consistent with the hypothesis of a short-time scale formation during the pre-stellar phase. We find a relative abundance ratio CHDOH/CHOD of 3.2 1.5. This result is consistent with a statistical deuteration. We cannot exclude H/D exchanges between water and methanol if water deuteration is of the order 0.1, as suggested by recent Herschel observations.
Accepted for publication in Astronomy & Astrophysics
References in corpus (5)
- Testing grain-surface chemistry in massive hot-core regions
- First detection of triply-deuterated methanol
- Decrease of the organic deuteration during the evolution of Sun-like protostars: the case of SVS13-A
- Millimeter Wave and Terahertz Spectra and Global Fit of Torsion-Rotation Transitions in the Ground, First and Second Excited Torsional States of 13CH3OH Methanol
- First detection of THz water maser in NGC7538-IRS1 with SOFIA and new 22 GHz e-MERLIN maps