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Detection of Water Vapor in the Terrestrial Planet Forming Region of a Transition Disk

Salyk, Colette and Lacy, John H. and Richter, Matthew J. and Zhang, Ke and Blake, Geoffrey A. and Pontoppidan, Klaus M. (2015) Detection of Water Vapor in the Terrestrial Planet Forming Region of a Transition Disk. Astrophysical Journal Letters, 810 (2). Art. No. L24. ISSN 2041-8205. https://resolver.caltech.edu/CaltechAUTHORS:20151207-092435300

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Abstract

We report a detection of water vapor in the protoplanetary disk around DoAr 44 with the Texas Echelon Cross Echelle Spectrograph—a visitor instrument on the Gemini north telescope. The DoAr 44 disk consists of an optically thick inner ring and outer disk, separated by a dust-cleared 36 AU gap, and has therefore been termed "pre-transitional." To date, this is the only disk with a large inner gap known to harbor detectable quantities of warm (T ~ 450 K) water vapor. In this work, we detect and spectrally resolve three mid-infrared pure rotational emission lines of water vapor from this source, and use the shapes of the emission lines to constrain the location of the water vapor. We find that the emission originates near 0.3 AU—the inner disk region. This characteristic region coincides with that inferred for both optically thick and thin thermal infrared dust emission, as well as rovibrational CO emission. The presence of water in the dust-depleted region implies substantial columns of hydrogen (>10^(22)cm^(-2) as the water vapor would otherwise be destroyed by photodissociation. Combined with the dust modeling, this column implies a gas/small-dust ratio in the optically thin dusty region of ≳ 1000. These results demonstrate that DoAr 44 has maintained similar physical and chemical conditions to classical protoplanetary disks in its terrestrial-planet forming regions, in spite of having formed a large gap.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/2041-8205/810/2/L24DOIArticle
http://iopscience.iop.org/article/10.1088/2041-8205/810/2/L24PublisherArticle
http://arxiv.org/abs/1508.07483arXivDiscussion Paper
ORCID:
AuthorORCID
Salyk, Colette0000-0003-3682-6632
Lacy, John H.0000-0001-6783-2328
Richter, Matthew J.0000-0002-8594-2122
Zhang, Ke0000-0002-0661-7517
Blake, Geoffrey A.0000-0003-0787-1610
Pontoppidan, Klaus M.0000-0001-7552-1562
Additional Information:© 2015 The American Astronomical Society. Received 2015 June 24; accepted 2015 August 6; published 2015 September 9. C.S. acknowledges helpful discussions with Joan Najita. Observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina).
Funders:
Funding AgencyGrant Number
NSFUNSPECIFIED
National Research Council of CanadaUNSPECIFIED
Comisión Nacional de Investigación Científica y Tecnológica (CONICYT)UNSPECIFIED
Australian Research CouncilUNSPECIFIED
Ministério da Ciência, Tecnologia e InovaçãoUNSPECIFIED
Ministerio de Ciencia, Tecnología e Innovación ProductivaUNSPECIFIED
Subject Keywords:protoplanetary disks; stars: pre-main sequence
Issue or Number:2
Record Number:CaltechAUTHORS:20151207-092435300
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20151207-092435300
Official Citation:Colette Salyk et al 2015 ApJ 810 L24
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:62638
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:08 Dec 2015 16:49
Last Modified:09 Dec 2019 21:54

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