Spitzer Infrared Spectrograph (IRS) observations of M, L, and T dwarfs

被引:66
作者
Roellig, TL
Van Cleve, JE
Sloan, GC
Wilson, JC
Saumon, D
Leggett, SK
Marley, MS
Cushing, MC
Kirkpatrick, JD
Mainzer, AK
Houck, JR
机构
[1] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[2] Ball Aerosp & Technol Corp, Boulder, CO 80301 USA
[3] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
[4] Univ Virginia, Charlottesville, VA 22903 USA
[5] Los Alamos Natl Lab, Div Appl Phys, Los Alamos, NM 87545 USA
[6] Joint Astron Ctr, Hilo, HI 96720 USA
[7] NASA, Ames Res Ctr, SETI Inst, Moffett Field, CA 94035 USA
[8] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA
[9] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
infrared : stars; stars; low-mass; brown dwarfs;
D O I
10.1086/421978
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first mid-infrared spectra of brown dwarfs, together with observations of a low-mass star. Our targets are the M3.5 dwarf GJ 1001A, the L8 dwarf DENIS-P J0255-4700, and the T1/T6 binary system epsilon Indi Ba/Bb. As expected, the mid-infrared spectral morphology of these objects changes rapidly with spectral class because of the changes in atmospheric chemistry resulting from their differing effective temperatures and atmospheric structures. By taking advantage of the unprecedented sensitivity of the Infrared Spectrograph on the Spitzer Space Telescope, we have detected the 7.8 mum methane and 10 mum ammonia bands for the first time in brown dwarf spectra.
引用
收藏
页码:418 / 421
页数:4
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