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Spectral energy distributions of T Tauri stars - Disk flaring and limits on accretion

Kenyon, S. J., Hartmann, L.·1987·The Astrophysical Journal

Abstract

The authors analyze spectral energy distributions of T Tauri stars (TTS) to place limits on disk accretion in this early phase of stellar evolution. The results reinforce the conclusion of Adams, Lada, and Shu that much of the infrared excess emission arises from reprocessing of stellar radiation by a dusty circumstellar disk. Observational constraints on disk geometries and disk masses are derived. The relative importance of accretion and solar-type chromospheric activity in T Tauri stars is assessed. The present analysis indicates that disk accretion in the T Tauri phase does not modify stellar evolution significantly and that the angular momentum of accreted material can be lost in a stellar wind.

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Metadata

Authors
Kenyon, S. J., & Hartmann, L.
Venue
The Astrophysical Journal
Published
1987-12
Volume
323
Pages
714
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2042484924
Cited by
697
References
0
FWCI
12.65
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Spectral energy distributions of T Tauri stars - Disk flaring and limits on accretion. https://app.cochat.ai/papers/10.1086/165866
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Kenyon, S. J., & Hartmann, L. (1987). Spectral energy distributions of T Tauri stars - Disk flaring and limits on accretion. The Astrophysical Journal. https://doi.org/10.1086/165866

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

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