Prof. Hayashi’s work on the evolution of stars in the pre-main sequence stage is reviewed. The historical background and the process of finding the Hayashi phase are mentioned. The work on the evolution of low-mass stars is also reviewed including the determination of the bottom of the main sequence and evolution of brown dwarfs, and comparison is made with the other works in the same period.
This content is only available via PDF.
© 2012 American Institute of Physics.
2012
American Institute of Physics
You do not currently have access to this content.