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Research on the Bottom of the Main Sequence and Brown Dwarfs in the Early Days
Published online by Cambridge University Press: 26 May 2016
Abstract
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One of the earliest works on the evolution of very low mass stars, Hayashi & Nakano (1963), is introduced, which determined self-consistently the bottom of the main sequence at 0.08M⊙ and investigated the evolution of an object of 0.05M⊙ from the stages with negligible electron degeneracy to those with high degeneracy.
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- Part 11. Summary
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- Copyright © Astronomical Society of the Pacific 2001
References
Hayashi, C., & Nakano, T.
1963, Progr. Theor. Phys., 30, 460
(HN63); or http://www-tap.scphys.kyoto-u.ac.jp/~nakano/member-e.html
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