articleThe Astrophysical JournalApr 15, 2005BRONZE OA

An Infrared Spectroscopic Sequence of M, L, and T Dwarfs

MCMichael C. CushingJTJohn T. RaynerWDWilliam D. Vacca

Ames Research Center · National Aeronautics and Space Administration · +2 more institutions

Indexed inarxivcrossrefdoaj

Abstract

We present a 0.6-4.1 micron spectroscopic sequence of M, L, and T dwarfs. The spectra have R~2000 from 0.9 to 2.4 microns and R=2500-200 from 2.9 to 4.1 microns. These new data nearly double the number of L and T dwarfs that have reported L-band spectra. The near-infrared spectra are combined with previously published red-optical spectra to extend the wavelength coverage to ~0.6 microns. Prominent atomic and molecular absorption features are identified including neutral lines of Al, Fe, Mg, Ca, Ti, Na, and K and 19 new weak CH_4 absorption features in the H-band spectra of mid- to late-type T dwarfs. In addition, we detect for the first time the 0-0 band of the A ^4\Pi - X ^4\Sigma^- transition of VO at ~1.06…

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Authors

3
  • MC
    Michael C. CushingCorresponding

    Ames Research Center, National Aeronautics and Space Administration, Search for Extraterrestrial Intelligence

  • JT
    John T. Rayner

    University of Hawaii System

  • WD
    William D. Vacca

    Ames Research Center, National Aeronautics and Space Administration

Topics & keywords

Keywords
  • Spectral line
  • Line (geometry)
  • Stellar classification
  • Infrared
  • Brown dwarf
  • Flux (metallurgy)
  • Absorption spectroscopy
  • Spectroscopy
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