Isabelle Baraffe, France Allard
Published 1997-05-12Version 1
Over the past decade considerable effort, both observational and theoretical, has been directed towards a more accurate determination of the stellar lower main sequence and of the sub-stellar domain covered by Brown Dwarfs and Planets. A review of the recent improvement in the theory of cool model atmospheres is presented.
Comments: 7 pages, Latex file, uses crckapb.sty, Proc. of IAU Symp 189, "Fundamental Stellar Properties...", eds T.R Bedding, A.J Booth and J. Davis, Kluwer
Rotation and variability of very low mass stars and brown dwarfs near Epsilon Ori
Formation and Evolution of Very Low Mass Stars and Brown Dwarfs
Low Mass Stars and Brown Dwarfs around Sigma Orionis
