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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

Takenori Nakano*
Affiliation:
c/o Department of Physics, Faculty of Science, Kyoto University, Kyoto 606-8502, Japan; E-mail: [email protected]

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.

Type
Part 11. Summary
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

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