English

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 \micron\micron) wavelength regimes. Important absorption bands and lines, including those of H2_2O, CH4_4, 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.

Keywords

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