A new model for brown dwarf spectra including accurate unified line shape theory for the Na I and K I resonance line profiles
A&A, 411 3 (2003) L473-L476
Published online: 2003-11-17
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Resonance potassium and sodium lines in the spectra of ultracool dwarfs
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Water vapour in the atmosphere of a transiting extrasolar planet
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Impact broadening of alkali lines in brown dwarfs
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The Physical Properties of HD 3651B: An Extrasolar Nemesis?
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The young, wide and very low mass visual binary Lambda Orionis 167
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