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TRANSITIONAL DISKS AS SIGNPOSTS OF YOUNG, MULTIPLANET SYSTEMS

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Dodson-Robinson, Sarah E., Salyk, Colette·2011·The Astrophysical Journal

Abstract

Although there has yet been no undisputed discovery of a still-forming planet embedded in a gaseous protoplanetary disk, the cleared inner holes of transitional disks may be signposts of young planets. Here, we show that the subset of accreting transitional disks with wide, optically thin inner holes of 15 AU or more can only be sculpted by multiple planets orbiting inside each hole. Multiplanet systems provide two key ingredients for explaining the origins of transitional disks. First, multiple planets can clear wide inner holes where single planets open only narrow gaps. Second, the confined, non-axisymmetric accretion flows produced by multiple planets provide a way for an arbitrary amount of mass transfer to occur through an apparently optically thin hole without overproducing infrared excess flux. Rather than assuming that the gas and dust in the hole are evenly and axisymmetrically distributed, one can construct an inner hole with apparently optically thin infrared fluxes by covering a macroscopic fraction of the hole's surface area with locally optically thick tidal tails. We also establish that other clearing mechanisms, such as photoevaporation, cannot explain our subset of accreting transitional disks with wide holes. Transitional disks are therefore high-value targets for observational searches for young planetary systems.

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Metadata

Authors
Dodson-Robinson, S. E., & Salyk, C.
Venue
The Astrophysical Journal
Published
2011-08-18
Volume
738
Issue
2
Pages
131
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2081836285
Cited by
216
References
5
FWCI
11.75
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: TRANSITIONAL DISKS AS SIGNPOSTS OF YOUNG, MULTIPLANET SYSTEMS. https://app.cochat.ai/papers/10.1088/0004-637x/738/2/131
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Dodson-Robinson, S. E., & Salyk, C. (2011). TRANSITIONAL DISKS AS SIGNPOSTS OF YOUNG, MULTIPLANET SYSTEMS. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/738/2/131

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