Beckman, John E.; Watt, Graeme D.; White, Glenn J.; Phillips, J. Peter; Frost, Robin L. and Davis, John H.
Detection of the 2(1,1) - 2(1,2) rotational emission line of HDO in the Orion Molecular Cloud.
Monthly Notices of the Royal Astronomical Society, 201
Full text available as:
Due to copyright restrictions, this file is not available for public download
The 2(1,1) - 2(1,2) rotational transition of HDO has been detected towards the KL position at the center of the OMC-1 at a velocity VLSR of +5.5(± 1.3)km s-1, corresponding to emission from the central core. This measurement is combined with previous estimates of the H2O abundance close to KL to obtain an [HDO]:[H2O] ratio of 9.5(±1.5) x 10-3. The systematic model-dependence of this ratio is examined in some detail, to show how reliably it may be used to obtain a radial gradient of [HDO]:[H2O], and hence of [D]:[H], within the Galaxy.
Actions (login may be required)