Abstract
We report the first detection of DCO+ in a circumstellar disk. The DCO+ J=5–4 line at 360.169 GHz is observed with the 15 m James Clerk Maxwell Telescope in the disk around the pre-main sequence star TW Hya. Together with measurements of the HCO+ and H13CO+ J=4–3 lines, this allows an accurate determination of the DCO+/HCO+ ratio in this disk. The inferred value of0.035±0.005 is close to that found in cold pre-stellar cores and is somewhat higher than that measured in the envelope around the low-mass proto star IRAS 16293-2422. It is also close to the DCN/HCN ratio obtained for pristine cometary material in the jet of comet Hale-Bopp. The observed DCO+/HCO+ ratio for TW Hya is consistent with theoretical models of disks which consider gas-phase fractionation processes within a realistic 2-D temperature distribution and which include the effects of freeze-out onto grains.
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van Dishoeck, E., Thi, WF. & van Zadelhoff, GJ. Detection of DCO+ in a circumstellar disk. Astrophysics and Space Science 285, 691–698 (2003). https://doi.org/10.1023/A:1026113327303
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DOI: https://doi.org/10.1023/A:1026113327303