Atmospheric Properties of Brown Dwarfs

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We present near-infrared spectra of 100 L dwarfs covering 0.8--2.5 microns obtained with the SpeX spectrograph on the IRTF telescope. We fit these data to synthetic spectra with a range of effective temperatures, gravities, and grain sedimentation efficiencies. >From this comparison, we investigate the range of physical properties spanned by the L dwarf spectral class.

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