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Black holes emerge when stellar cores implode during supernova events. While a star's outer shell violently expands into space, its deepest internal components collapse inward, concentrating a portion of the star's substance into either a black hole or, for less massive stars, a neutron star. Since stellar mass boundaries remain undefined, one might assume black hole mass distribution would taper off gradually without distinct interruptions.,推荐阅读快连下载获取更多信息
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