SIMBAD references

2003ApJ...594..510B - Astrophys. J., 594, 510-524 (2003/September-1)

The spectra of T dwarfs. II. Red optical data.


Abstract (from CDS):

We present 6300-10100 Å spectra for a sample of 13 T dwarfs observed using LRIS mountedtpdel 99 on the Keck I 10 m Telescope. A variety of features are identified and analyzed, including pressure-broadened K I and Na I doublets; narrow Cs I and Rb I lines; weak CaH, CrH, and FeH bands; strong H2O absorption; and a possible weak CH4 band. Hα emission is detected in three of the T dwarfs, strong in the previously reported active T dwarf 2MASS 1237+6526 and weak in SDSS 1254-0122 and 2MASS 1047+2124. None of the T dwarfs exhibit Li I absorption. Guided by the evolution of optical spectral features with near-infrared spectral type, we derive a parallel optical classification scheme, focusing on spectral types T5 to T8, anchored to select spectral standards. We find general agreement between optical and near-infrared types for nearly all the T dwarfs so far observed, including two earlier type T dwarfs, within our classification uncertainties (∼1 subtype). These results suggest that competing gravity and temperature effects compensate for each other over the 0.6-2.5 µm spectral region. We identify one possible means of disentangling these effects by comparing the strength of the K I red wing to the 9250 Å H2O band. One of our objects, 2MASS 0937+2931, exhibits a peculiar spectrum with a substantial red slope and relatively strong FeH absorption, both consequences of a metal-deficient atmosphere. On the basis of its near-infrared properties and substantial space motion, this object may be a thick disk or halo brown dwarf.

Abstract Copyright:

Journal keyword(s): Stars: Activity - Stars: Fundamental Parameters - Stars: Individual: Alphanumeric: 2MASS J09373487+2931409 - Stars: Low-Mass, Brown Dwarfs

Simbad objects: 33

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2003ApJ...594..510B and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact