2MASS J22521073-1730134: A resolved L/T binary at 14 parsecs

被引:67
|
作者
Reid, IN
Lewitus, E
Burgasser, AJ
Cruz, KL
机构
[1] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[2] Amer Museum Nat Hist, Dept Astrophys, New York, NY 10024 USA
来源
ASTROPHYSICAL JOURNAL | 2006年 / 639卷 / 02期
关键词
binaries : visual; stars : individual (2MASSW J22521073-1730134) stars : low-mass; brown dwarfs;
D O I
10.1086/499484
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
NICMOS images of the nearby late-type L dwarf 2MASS J22521073 - 1730134 ( DENIS- P J225210.73 - 173013.4) show that it is a close double, separation 0".13. The companion is 1.0 mag fainter than the primary in the F110W passband and 1.55 mag fainter in the F170M images. The latter passband is centered on the 1.6 mu m methane band. The small separation and the absence of an optical counterpart suggest that the two sources are associated; the relatively blue infrared color suggests that 2MASS J22521073 - 1730134B is a T-type binary companion of the late-L primary. This hypothesis is supported by infrared spectroscopy, which shows weak methane absorption in both the H and K passbands. We estimate a distance of 13: 6(-2.6)(+3.8) pc to the system and a projected linear separation of 1.75 AU. We consider the potential for measuring dynamical masses of the two components.
引用
收藏
页码:1114 / 1119
页数:6
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