Evolutionary Models for Very Low‐Mass Stars and Brown Dwarfs with Dusty Atmospheres
Evolutionary Models for Very Low‐Mass Stars and Brown Dwarfs with Dusty Atmospheres
We present evolutionary calculations for very-low-mass stars and brown dwarfs based on synthetic spectra and non-grey atmosphere models which include dust formation and opacity, i.e. objects with $\te\simle 2800$ K. The interior of the most massive brown dwarfs is shown to develop a conductive core after $\sim 2$ Gyr which …