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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
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