In this contribution, I review a subset of our recent efforts in spectral and opacity modeling aimed at guiding the study of brown dwarfs, L dwarfs, and T dwarfs. I discuss theoretical calculations of the alkali line profiles, newly generated CrH opacities, new evidence for refractory rainout in T dwarfs from optical spectral measurements, and the controversy concerning the distinction between brown dwarfs and planets.
CITATION STYLE
Burrows, A. (2003). Modeling Brown Dwarfs, L Dwarfs, and T Dwarfs. Symposium - International Astronomical Union, 211, 393–402. https://doi.org/10.1017/s007418090021098x
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