NGC 2264, NGC 2547 and NGC 2516 stellar radii
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Rapidly rotating, low-mass members of eclipsing binary systems have measured radii that are significantly larger than predicted by standard evolutionary models. It has been...
食双星系统（eclipsing binary system）中快速旋转的低质量成员星，其测得的半径显著大于标准演化模型（standard evolutionary model）的理论预言值。目前已有……
