Radial velocities for 16 hot Jupiter host stars
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/84c6bb64-3607-54ba-ba2f-604da4ac9113
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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...
