H and K Band Methane Features in an L Dwarf, 2MASS 0920+35
arXiv:astro-ph/0109370 · doi:10.1086/324440
Abstract
We have obtained near-infrared spectra of three L dwarfs discovered by 2MASS, 1506+13 (L3), 1507-16 (L5), and 0920+35 (L6.5). From the comparison of the H and K band spectra of these L dwarfs, we have found the presence of methane absorption in 0920+35. This implies that detectable methane absorption in the H and K bands, usually considered the signature of a T dwarf, can be present in objects classified optically as late L. Methane detection in L dwarfs is consistent with the presence of a dust layer deep in the atmosphere as the unified model of Tsuji suggests.
Accepted for publication in ApJ Letters; 8 pages, 4 figures
References in corpus (1)
Cited by in corpus (13)
- An Infrared Spectroscopic Sequence of M, L and T Dwarfs
- A Unified Near Infrared Spectral Classification Scheme for T Dwarfs
- The NIRSPEC Brown Dwarf Spectroscopic Survey. I. Low-Resolution Near-Infrared Spectra
- Multiplicity of Nearby Free-floating Ultra-cool Dwarfs: a HST-WFPC2 search for companions
- The Spectra of T Dwarfs. II. Red Optical Data
- Dust in the Photospheric Environment: Unified Cloudy Models of M, L, and T Dwarfs
- SDSS J1534+1615AB: A Novel T Dwarf Binary Found with Keck Laser Guide Star Adaptive Optics and the Potential Role of Binarity in the L/T Transition
- Dust in the Photospheric Environment II. Effect on the Near Infrared Spectra of L and T Dwarfs
- Spectral Classification and Effective Temperatures of L and T Dwarfs Based of Near-Infrared Spectra
- A Signature of Chromospheric Activity in Brown Dwarfs Revealed by 2.5-5.0 Micron AKARI Spectra
- 2MASS J03105986+1648155AB - A new binary at the L/T transition
- Correlated spectral variability in brown dwarfs
- Effect of Dust Size on the Near-Infrared Spectra (1.0-5.0 m) of Brown Dwarf Atmospheres