HARPS radial velocity follow up of TOI-1634
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Studies of close-in planets orbiting M dwarfs have suggested that the M-dwarf radius valley may be well explained by distinct formation timescales between enveloped terrestrials...
针对环绕M型矮星（M dwarfs）的近距离系外行星的相关研究表明，M矮星半径谷（M-dwarf radius valley）或可通过带有包层的类地行星之间迥异的形成时标得到合理解释……
