DISCOVERY OF THE COLDEST IMAGED COMPANION OF A SUN-LIKE STAR
DISCOVERY OF THE COLDEST IMAGED COMPANION OF A SUN-LIKE STAR
复制标题
类太阳恒星最冷的伴星图像的发现
DOI:
10.1088/0004-637x/707/2/l123
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发表时间:
2009
期刊:
影响因子:
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通讯作者:
U. Hawaii
中科院分区:
文献类型:
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作者:
C. Thalmann;J. Carson;M. Janson;M. Goto;M. McElwain;S. Egner;M. Feldt;J. Hashimoto;Y. Hayano;T. Henning;K. Hodapp;R. Kandori;H. Klahr;T. Kudo;N. Kusakabe;C. Mordasini;J. Morino;H. Suto;R. Suzuki;Motohide Tamura Max Planck Institute for Astronomy;College of Charleston;U. Toronto;P. University;Subaru Telescope;N. A. O. Japan;Institute for Astronomy;U. Hawaii
We present the discovery of a brown dwarf or possible planet at a projected separation of 1.″9 = 29 AU around the star GJ 758, placing it between the separations at which substellar companions are expected to form by core accretion (∼5 AU) or direct gravitational collapse (typically ≳100 AU). The object was detected by direct imaging of its thermal glow with Subaru/HiCIAO. At 10–40 times the mass of Jupiter and a temperature of 550–640 K, GJ 758 B constitutes one of the few known T-type companions, and the coldest ever to be imaged in thermal light around a Sun-like star. Its orbit is likely eccentric and of a size comparable to Pluto's orbit, possibly as a result of gravitational scattering or outward migration. A candidate second companion is detected at 1.″2 at one epoch.