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High-Resolution Spectroscopic Surveys of Ultracool Dwarf Stars & Brown Dwarfs

Published onMay 31, 2019
High-Resolution Spectroscopic Surveys of Ultracool Dwarf Stars & Brown Dwarfs
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Abstract

High resolution spectroscopy of the lowest-mass stars and brown dwarfs reveals their origins, multiplicity, compositions and physical properties, with implications for the star formation and chemical evolution history of the Milky Way. We motivate the need for high-resolution, infrared spectroscopic surveys to reach theses faint sources.

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