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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
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
Information
Symposium - International Astronomical Union , Volume 211: Brown Dwarfs , 2003 , pp. 551 - 552
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Hayashi, C. 1961, PASJ, 13, 450 Google Scholar
Hayashi, C., & Nakano, T. 1963, Progr. Theor. Phys., 30, 460 (HN63); or http://www-tap.scphys.kyoto-u.ac.jp/~nakano/member-e.html Google Scholar
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