An Infrared Spectroscopic Sequence of M, L, and T Dwarfs
Ames Research Center · National Aeronautics and Space Administration · +2 more institutions
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…
Citation impact
- FWCI
- 17.25
- Percentile
- 100%
- References
- 84
Authors
3- MCMichael C. CushingCorresponding
Ames Research Center, National Aeronautics and Space Administration, Search for Extraterrestrial Intelligence
- JTJohn T. Rayner
University of Hawaii System
- WDWilliam D. Vacca
Ames Research Center, National Aeronautics and Space Administration
Topics & keywords
- Spectral line
- Line (geometry)
- Stellar classification
- Infrared
- Brown dwarf
- Flux (metallurgy)
- Absorption spectroscopy
- Spectroscopy