NGC 4349 127 RV and activity indices
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Several evolved stars have been found to exhibit long-period radial velocity variations that cannot be explained by planetary or brown dwarf companions. Non-radial oscillations...
已有研究在多颗已演化恒星中发现其存在长周期视向速度变化,此类变化无法通过行星或褐矮星伴星的作用加以解释。非径向振荡……



