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astro-ph2000
The use of the NEXTGEN model atmospheres for cool giants in a light curve synthesis code
Jerome A. Orosz, Peter H. Hauschildt
We have written a light curve synthesis code that makes direct use of model atmosphere specific intensities, in particular the NEXTGEN model atmosphere grid for cool giants (T_eff…
astro-ph2000
Pre-Main Sequence models for low-mass stars and brown dwarfs
I. Baraffe, G. Chabrier, F. Allard +1
We present evolutionary models for low mass stars and brown dwarfs ($m \le 1.2 \msol$) based on recent improvement of the theory: equation of state, atmosphere models, ... We conce…