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Cited by 388

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Accretion disks around T Tauri stars

Bertout, Claude, Basri, Gibor, Bouvier, Jerome·1988·The Astrophysical Journal

Abstract

The authors examine the proposition that many T Tauri stars are still actively accreting material from a surrounding disk of material formed at the same time as the star. It is shown that the observations are both unified and explained if classical T Tauri stars are chromospherically active pre-main-sequence stars with accretion disks. Contemporaneous optical and ultraviolet observations, along with extensive photometric monitoring in the optical and infrared, are used to test disk models and to show that there is evidence for accretion in the range 5×10-8 - 5×10-7M_sun;yr-1 from stars exhibiting strong ultraviolet excesses. These models also explain the infrared spectrum shortward of 10 μm and the total system luminosities.

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Metadata

Authors
Bertout, C., Basri, G., & Bouvier, J.
Venue
The Astrophysical Journal
Published
1988-07
Volume
330
Pages
350
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2042336801
Cited by
388
References
0
FWCI
23.48
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Accretion disks around T Tauri stars. https://app.cochat.ai/papers/10.1086/166476
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Bertout, C., Basri, G., & Bouvier, J. (1988). Accretion disks around T Tauri stars. The Astrophysical Journal. https://doi.org/10.1086/166476

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