Brown dwarf in neighbouring solar system is actually a spinning duo

成果类型:
Article
署名作者:
Xuan, Jerry W.; Oppenheimer, Rebecca
署名单位:
California Institute of Technology; American Museum of Natural History (AMNH)
刊物名称:
Nature
ISSN/ISSBN:
0028-2491
DOI:
10.1038/d41586-024-03501-3
发表日期:
2025-01-23
关键词:
unconventional superconductivity moire STATES mott TRANSITION physics MODEL
摘要:
The nearby star Gliese 229 harbours a 'brown dwarf' companion: an object less massive than a star but more massive than a planet. High-resolution observations reveal that it is two objects, each about 30 times the mass of Jupiter, that circle one another every 12 days as they orbit their sun every few hundred years.