A giant planet candidate near a young brown dwarf - Direct VLT/NACO observations using IR wavefront sensing

被引:488
作者
Chauvin, G
Lagrange, AM
Dumas, C
Zuckerman, B
Mouillet, D
Song, I
Beuzit, JL
Lowrance, P
机构
[1] European So Observ, Santiago 19, Chile
[2] Observ Grenoble, Astrophys Lab, St Martin Dheres, France
[3] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[4] Univ Calif Los Angeles, Ctr Astrobiol, Los Angeles, CA 90095 USA
[5] Observ Midi Pyrenees, Astrophys Lab, Tarbes, France
[6] CALTECH, Ctr Infrared Proc & Anal, Spitzer Sci Ctr, Pasadena, CA 91125 USA
关键词
2MASSWJ; 1207334-393254; brown dwarf; giant planet; adaptive optics imaging and spectroscopy;
D O I
10.1051/0004-6361:200400056
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present deep VLT/NACO infrared imaging and spectroscopic observations of the brown dwarf 2MASSWJ 1207334-393254, obtained during our on-going adaptive optics survey of southern young, nearby associations. This similar to25 M-Jup brown dwarf, located similar to70 pc from Earth, has been recently identified as a member of the TW Hydrae Association (age similar to 8 Myr). Using adaptive optics infrared wavefront sensing to acquire sharp images of its circurnstellar environment, we discovered a very faint and very red object at a close separation of similar to780 mas (similar to55 AU). Photometry in the H, K-s and L' bands and upper limit in J-band are compatible with a spectral type L5-L9.5. Near-infrared spectroscopy is consistent with this spectral type estimate. Different evolutionary models predict an object within the planetary regime with a mass of M = 5 +/- 2 M-Jup and an effective temperature of T-eff = 1250 +/- 200 K.
引用
收藏
页码:L29 / L32
页数:4
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