"This neutron star was born so hot that nuclear fusion happened on its surface, producing a carbon atmosphere just 10 centimetres thick."
这颗中子星产生时温度如此之高，其表面还在进行核子融合，从而产生了只有10厘米厚的碳大气层。
And if the axis of rotation doesn't coincide with the line through the two hot spots, if the neutron star rotates, you're going to see X-ray pulsations.
不合这两点之间的线，相一致，如果中子星旋转，你会看到x射线脉动，当热点在这里。
This neutron star was born so hot that nuclear fusion happened on its surface, producing a carbon atmosphere just 10 centimeters thick.
阿尔伯塔大学的天文学家克雷格.汉克在新闻稿中写道，“这颗中子星诞生时表面温度非常之高，以至于在它的表面也可以发生核聚变，并产生了大约10厘米厚的碳质云层。”
This neutron star was born so hot that nuclear fusion happened on its surface, producing a carbon atmosphere just 10 centimeters thick.
阿尔伯塔大学的天文学家克雷格.汉克在新闻稿中写道，“这颗中子星诞生时表面温度非常之高，以至于在它的表面也可以发生核聚变，并产生了大约10厘米厚的碳质云层。”
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