paper

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

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