SPATIALLY RESOLVED SPECTROSCOPY OF THE EXOPLANET HR 8799 c

被引:82
作者
Janson, M. [1 ]
Bergfors, C. [2 ]
Goto, M. [2 ]
Brandner, W. [2 ]
Lafreniere, D. [3 ]
机构
[1] Univ Toronto, Toronto, ON, Canada
[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[3] Univ Montreal, Montreal, PQ, Canada
关键词
planetary systems; techniques: spectroscopic; INTEGRAL FIELD SPECTROSCOPY; EVOLUTIONARY MODELS; BROWN DWARFS; PLANET; ATMOSPHERES; COMPANION; CONTRAST; SYSTEM; STARS; EARTH;
D O I
10.1088/2041-8205/710/1/L35
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
HR 8799 is a multi-planet system detected in direct imaging, with three companions known so far. Here, we present spatially resolved Very Large Telescope/NACO 3.88-4.10 mu m spectroscopy of the middle planet, HR 8799 c, which has an estimated mass of similar to 1.0 M-Jup, temperature of similar to 1100 K, and projected separation of 38 AU. The spectrum shows some differences in the continuum from existing theoretical models, particularly longwards of 4 mu m, implying that detailed cloud structure or non-equilibrium conditions may play an important role in the physics of young exoplanetary atmospheres.
引用
收藏
页码:L35 / L38
页数:4
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