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A Near-Infrared Spectral Sequence of Late M, L, and T Dwarfs
Published online by Cambridge University Press: 26 May 2016
Abstract
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We present the initial results of a medium resolution, 0.8 to 4.2 μm spectroscopic survey of M, L, and T dwarfs. We have identified the most prominent molecular and atomic absorption features found in the spectra of these late-type dwarfs. We have also compared the spectra to a laboratory FeH emission spectrum and identified nearly 100 features common to the FeH spectrum and the dwarf spectra from 0.99 to 1.8 μm.
- Type
- Part 7. Atmospheres and Internal Structure
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- Copyright
- Copyright © Astronomical Society of the Pacific 2001
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