Fast-rotating M-dwarf stars in NGC 2547
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At fast rotation rates, the coronal activity of G- and K-type stars has been observed to "saturate" and then decline again at even faster rotation rates - a phenomenon dubbed...
当恒星处于快速自转状态时，观测发现G型和K型恒星的日冕活动会先进入"饱和"阶段，随后在自转速率进一步加快时再次回落——这一现象被称为……
