The Spectra and Classification of L and T Dwarfs
Astrophysics
2007-05-23 v1
Abstract
In this contribution, I discuss some of the salient features of L and T dwarf spectra in both the red optical (6300--10000 {\AA}) and near-infrared (1--2.5 ) wavelength regimes. Important absorption bands and lines, including those of HO, CH, FeH, CrH, CO, and the alkali metal lines, are identified, and the development of recent classification schemes based on these features are discussed. I briefly point out future work required in these wavelength regions and in the mid-infrared that are required to garner a complete picture of these low-luminosity dwarfs.
Cite
@article{arxiv.astro-ph/0109422,
title = {The Spectra and Classification of L and T Dwarfs},
author = {Adam J. Burgasser},
journal= {arXiv preprint arXiv:astro-ph/0109422},
year = {2007}
}
Comments
10 pages, 6 figures, To be published in Proceedings of the 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun