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Supersonic Convection and the Structure of T-Tauri Stars

Published online by Cambridge University Press:  25 April 2016

A. J. R. Prentice
A. J. R. Prentice*
Affiliation:
Mathematics Department, Monash University
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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).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 3 , October 1972 , pp. 152 - 153
Copyright
Copyright © Astronomical Society of Australia 1972

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References

1 Ambartzumian, V. A., Astr. Zh., 26, 3 (1949).Google Scholar
2 Herbig, G. H., Adv. Astr. Astophys. 1, 47 (1962).CrossRefGoogle Scholar
3 Hayashi, C., Pub. Astr. Soc. Japan, 13, 450 (1961).Google Scholar