Research on the Bottom of the Main Sequence and Brown Dwarfs in the Early Days

Details Research on the Bottom of the Main Sequence and Brown Dwarfs in the Early Days Research on the Bottom of the Main Sequence and Brown Dwarfs in the Early Days

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003iaus..211..551n&link_type=abstract

Brown Dwarfs, Proceedings of IAU Symposium #211, held 20-24 May 2002 at University of Hawaii, Honolulu, Hawaii. Edited by Eduard

Astronomy and Astrophysics

Astronomy

Scientific paper

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 0.08 M&sun; and investigated the evolution of an object of 0.05 M&sun; from the stages with negligible electron degeneracy to those with high degeneracy.

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