Radial velocities for 16 hot Jupiter host stars
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We provide evidence that the obliquities of stars with close-in giant planets were initially nearly random, and that the low obliquities that are often observed are a...
本研究提供证据表明，拥有近距离巨行星的恒星自转轴倾角（obliquity）初始时近乎随机分布，而常被观测到的低倾角现象则为……
