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Survey of Cold Water Lines in Protoplanetary Disks: Indications of Systematic Volatile Depletion
Date
2017-06-01
Author
Du, Fujun
Bergin, Edwin Anthony
Hogerheijde, Michiel
van Dishoeck, Ewine F.
Blake, Geoff
Bruderer, Simon
Cleeves, Ilse
Dominik, Carsten
Fedele, Davide
Lis, Dariusz C.
Melnick, Gary
Neufeld, David
Pearson, John
Yıldız, Umut
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We performed very deep searches for 2 ground-state water transitions in 13 protoplanetary disks with the HIFI instrument on board the Herschel Space Observatory, with integration times up to 12 hr per line. We also searched for, with shallower integrations, two other water transitions that sample warmer gas. The detection rate is low, and the upper limits provided by the observations are generally much lower than predictions of thermo-chemical models with canonical inputs. One ground-state transition is newly detected in the stacked spectrum of AA. Tau, DM. Tau, LkCa. 15, and MWC. 480. We run a grid of models to show that the abundance of gas-phase oxygen needs to be reduced by a factor of at least similar to 100 to be consistent with the observational upper limits (and positive detections) if a dust-to-gas mass ratio of 0.01 were to be assumed. As a continuation of previous ideas, we propose that the underlying reason for the depletion of oxygen (hence the low detection rate) is the freeze-out of volatiles such as water and CO onto dust grains followed by grain growth and settling/migration, which permanently removes these gas-phase molecules from the emissive upper layers of the outer disk. Such depletion of volatiles is likely ubiquitous among different disks, though not necessarily to the same degree. The volatiles might be returned back to the gas phase in the inner disk (less than or similar to 15 au), which is consistent with current constraints. Comparison with studies on disk dispersal due to photoevaporation indicates that the timescale for volatile depletion is shorter than that of photoevaporation.
URI
https://hdl.handle.net/11511/115943
Journal
ASTROPHYSICAL JOURNAL
DOI
https://doi.org/10.3847/1538-4357/aa70ee
Collections
Department of Physics, Article
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BibTeX
F. Du et al., “Survey of Cold Water Lines in Protoplanetary Disks: Indications of Systematic Volatile Depletion,”
ASTROPHYSICAL JOURNAL
, vol. 842, no. 2, pp. 0–0, 2017, Accessed: 00, 2025. [Online]. Available: https://hdl.handle.net/11511/115943.