post-core-collapse cluster 核心坍缩后星团
core-collapse supernova 核塌缩超新星爆炸
post-core-collapse e cluster 核心坍缩后星团
The deciding factors for whether a core collapse produces a GRB appear to be the mass and rotation rate of the progenitor star at the time of its death.
核心坍塌是否能产生GRB的关键因素,似乎在于原来恒星临终时的质量与转动速率。
The white source near the center of the image is a dense, rapidly rotating neutron star, or pulsar, all that remains of a core-collapse supernova explosion.
图片靠近中心部分的白色光源为一种密度大,急速旋转的中子星,或是脉冲星--都是核心坍缩的超新星爆炸的残留物。
They come in two types, long and short, with the former the most common and thought to be caused by the core-collapse of a supernova.
伽马射线爆有长时间的和短时间的两种,其中据信由超新星核的坍塌引起的长时间伽马射线爆是最常见的。
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