The abundance of H2O and HDO in Orion KL from Herschel/HIFI

Justin L. Neill; Shiya Wang; Edwin A. Bergin; Nathan R. Crockett; Cécile Favre; René Plume; Gary J. Melnick

doi:10.1088/0004-637X/770/2/142

paper

The abundance of H2O and HDO in Orion KL from Herschel/HIFI

arXiv:1305.2247 · doi:10.1088/0004-637X/770/2/142

Abstract

Using a broadband, high spectral resolution survey toward Orion KL acquired with Herschel/HIFI as part of the HEXOS key program, we derive the abundances of H $_{2}$ O and HDO in the different spatial/velocity components associated with this massive star-forming region: the Hot Core, Compact Ridge, and Plateau. A total of 20 transitions of H $_{2}$ $^{18}$ O, 14 of H $_{2}$ $^{17}$ O, 37 of HD $^{16}$ O, 6 of HD $^{18}$ O, and 6 of D $_{2}$ O are used in the analysis, spanning from ground state transitions to over 1200 K in upper-state energy. Low-excitation lines are detected in multiple components, but the highest-excitation lines ( $E_{u} >$ 500 K) are well modeled as emitting from a small ( $\sim 2"$ ) clump with a high abundance of H $_{2}$ O ( $χ = 6.5 \times 1 0^{- 4}$ relative to H $_{2}$ ) and a HDO/H $_{2}$ O ratio of 0.003. Using high spatial resolution ( $1.5" \times 1.1"$ ) images of two transitions of HDO measured by ALMA as part of its science verification phase, we identify this component as located near, but not directly coincident with, known continuum sources in the Hot Core region. Significant HDO/H $_{2}$ O fractionation is also seen in the Compact Ridge and Plateau components. The outflowing gas, observed with both emission and absorption components, has a lower HDO/H $_{2}$ O ratio than the compact components in Orion KL, which we propose could be due to modification by gas-phase shock chemistry.

39 pages, 11 figures, 6 tables. Accepted to ApJ

The abundance of H2O and HDO in Orion KL from Herschel/HIFI

Abstract

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