因为AGB超星风仅仅发生在AGB的最后阶段，所以在超星风发生重要作用之前，中等质量AGB的简并核可以达到钱德拉塞卡极限。
Since AGB superwind only occurs at the final stage of AGB stars, it may allow the degenerate core of intermediate-mass AGB star to reach the Chandresekhar mass before the AGB superwind.
当一颗白矮星以这种方式增长到足够的质量时，它将达到钱德拉·塞卡极限。
When a White Dwarf takes on enough mass in this manner, it reaches a level called the chandrasekhar limit.
这幅组合图像显示了钱德拉·塞卡北深空区的一小部分。
This composite image shows a small region of the ChandraDeep Field North.
当一颗白矮星以这种方式增长到足够的质量时，它将达到一个称为钱德拉·塞卡极限的质量标准。
When a White Dwarf takes on enough mass in this manner it reaches a level called the chandrasekhar limit.
我已经要求科技部举办一个国家级的庆典，以庆祝我们20世纪卓越的科学家钱德拉·塞卡教授的百年诞辰。
I have asked our the Ministry of Science and Technology to undertake a national celebration of the birth centenary of Professor S.Chandrasekhar, one of the outstanding scientists of the 20th century.
塔塔咨询的首席执行官纳塔拉詹•钱德拉·塞卡兰(Natarajan Chandrasekaran)在过去三个月里访问了遍布世界各地的100多个客户，并表示他们坚决果断。
Natarajan Chandrasekaran, TCS's chief executive, has visited more than 100 customers worldwide in the past three months and says they are resolute.
最终中子恒星中暗物质恒星的质量会超过它的“钱德拉·塞卡极限(Chandrashekar limit)——超过了这个极限值，一个恒星就经受不住引力所引起的压力。”
Eventually, the mass of the dark matter star would exceed its "Chandrashekar limit" - beyond which a star cannot withstand gravitational pressure.
最终中子恒星中暗物质恒星的质量会超过它的“钱德拉·塞卡极限(Chandrashekar limit)——超过了这个极限值，一个恒星就经受不住引力所引起的压力。”
Eventually, the mass of the dark matter star would exceed its "Chandrashekar limit" - beyond which a star cannot withstand gravitational pressure.
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