Supersonic Convection and the Structure of T-Tauri Stars
Abstract
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).
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- October 1972
- DOI:
- 10.1017/S1323358000013369
- Bibcode:
- 1972PASA....2..152P