Theoretical modelling of optical and IR spectra of brown dwarfs and ultracool dwarfs

Astronomy and Astrophysics – Astronomy

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Stars: Low-Mass, Brown Dwarfs, Stars: Evolution, Synthetical Spectra

Scientific paper

The current state of theoretical modelling of the spectra of cool dwarfs and ultracool objects are discussed. Fits of synthetical spectral energy distributions (SEDs) in the optical and IR spectral regions to observed spectra show problems of theoretical modelling. Problems of interpretation of observed spectra are more obvious for the case of L and T dwarfs. Still even for late-M dwarfs the situation is far from being perfect. Some examples of the fine analysis of the spectra of ultracool dwarfs are presented.

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