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Spectral Energy Distributions of T Tauri Stars with Passive Circumstellar Disks

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Chiang, E. I., Goldreich, P.·1997·The Astrophysical Journal

Abstract

We derive hydrostatic, radiative equilibrium models for passive disks surrounding T Tauri stars. Each disk is encased by an optically thin layer of superheated dust grains. This layer reemits directly to space about half the stellar energy it absorbs. The other half is emitted inward and regulates the interior temperature of the disk. The heated disk flares. As a consequence, it absorbs more stellar radiation, especially at large radii, than a flat disk would. The portion of the spectral energy distribution contributed by the disk is fairly flat throughout the thermal infrared. At fixed frequency, the contribution from the surface layer exceeds that from the interior by about a factor 3 and is emitted at more than an order of magnitude greater radius. Spectral features from dust grains in the superheated layer appear in emission if the disk is viewed nearly face-on.

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Metadata

Authors
Chiang, E. I., & Goldreich, P.
Venue
The Astrophysical Journal
Published
1997-11-20
Volume
490
Issue
1
Pages
368-376
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2099559854
Cited by
1,683
References
0
FWCI
12.17
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Spectral Energy Distributions of T Tauri Stars with Passive Circumstellar Disks. https://app.cochat.ai/papers/10.1086/304869
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Chiang, E. I., & Goldreich, P. (1997). Spectral Energy Distributions of T Tauri Stars with Passive Circumstellar Disks. The Astrophysical Journal. https://doi.org/10.1086/304869

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.