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Comparison of the dust and gas radial structure in the transition disk [PZ99] J160421.7-213028

Zhang, Ke and Isella, Andrea and Carpenter, John M. and Blake, Geoffrey A. (2014) Comparison of the dust and gas radial structure in the transition disk [PZ99] J160421.7-213028. Astrophysical Journal, 791 (1). Art. No. 42. ISSN 0004-637X. doi:10.1088/0004-637X/791/1/42. https://resolver.caltech.edu/CaltechAUTHORS:20140714-085408641

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Abstract

We present ALMA observations of the 880  μm continuum and CO J = 3–2 line emission from the transition disk around [PZ99] J160421.7-213028, a solar mass star in the Upper Scorpius OB association. Analysis of the continuum data indicates that 80% of the dust mass is concentrated in an annulus extending between 79 and 114 AU in radius. Dust is robustly detected inside the annulus, at a mass surface density 100 times lower than that at 80 AU. The CO emission in the inner disk also shows a significantly decreased mass surface density, but we infer a cavity radius of only 31 AU for the gas. The large separation of the dust and gas cavity edges, as well as the high radial concentration of millimeter-sized dust grains, is qualitatively consistent with the predictions of pressure trap models that include hydrodynamical disk–planet interactions and dust coagulation/fragmentation processes.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/791/1/42DOIArticle
http://iopscience.iop.org/0004-637X/791/1/42/articlePublisherArticle
http://arxiv.org/abs/1406.6974arXivArticle
ORCID:
AuthorORCID
Zhang, Ke0000-0002-0661-7517
Isella, Andrea0000-0001-8061-2207
Carpenter, John M.0000-0003-2251-0602
Blake, Geoffrey A.0000-0003-0787-1610
Additional Information:© 2014 The American Astronomical Society. Received 2014 April 18; accepted 2014 June 25; published 2014 July 24. We thank Crystal Brogan and Steve Myers for their assistance with the data reduction. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00526.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. A.I. and J.M.C. acknowledge support from NSF awards AST-1109334 and AST-1140063. K.Z. and G.A.B. gratefully acknowledge funding provided by NSF award AST-1109857 and NASA grant NNX11AK86G.
Funders:
Funding AgencyGrant Number
NSFAST-1109334
NSFAST-1140063
NSFAST-1109857
NASANNX11AK86G
Subject Keywords:protoplanetary disks; stars: pre-main sequence; submillimeter: stars
Issue or Number:1
DOI:10.1088/0004-637X/791/1/42
Record Number:CaltechAUTHORS:20140714-085408641
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140714-085408641
Official Citation:Comparison of the Dust and Gas Radial Structure in the Transition Disk [PZ99] J160421.7-213028 Ke Zhang et al. 2014 ApJ 791 42
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:47158
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:14 Jul 2014 19:40
Last Modified:10 Nov 2021 17:35

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