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Supersonic Convection and the Structure of T-Tauri Stars
Published online by Cambridge University Press: 25 April 2016
Extract
It is generally agreed that T-Tauri stars are very young stars of solar mass which are still engaged in the process of gravitational contraction toward the main sequence (Ambartzumian, Herbig).
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- Information
- Publications of the Astronomical Society of Australia , Volume 2 , Issue 3 , October 1972 , pp. 152 - 153
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- Copyright © Astronomical Society of Australia 1972
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