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n. (Chandrasekhar)人名；（印、英）钱德拉塞卡尔
1、When a White Dwarf takes on enough mass in this manner, it reaches a level called the chandrasekhar limit.───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。
2、In 1930, the physicist Chandrasekhar predicted that white dwarfs could not exist if their mass is larger than 1. 4 solar mass.───预测白矮星的质量，若大于太阳的1。4倍，就不能存在，它是个。
3、When a white dwarf takes on enough mass in this manner it reaches a level called the chandrasekhar limit.───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。
4、An argument about white dwarfs between Eddington and Chandrasekhar and its inspiration───爱丁顿、钱德拉塞卡关于白矮星的争论及其启示
5、K. M. Chandrasekhar, cabinet secretary, says the key is raising abysmal agricultural productivity.───印度政府内阁部长K•M•钱德拉塞卡 (K M Chandrasekhar)表示，提高印度极为低下的农业生产率是关键。
6、When a White Dwarf takes on enough mass in this manner it reaches a level called the chandrasekhar limit.───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。
7、who is new to our country, knows more about our history than you do.───是初来步到，但他认识本国历史比你们还多。
1、Theory predicts that a white dwarf star will explode when infalling matter from a companion star increases the mass of the white dwarf beyond a critical mass limit, known as the Chandrasekhar limit.
2、An account of an argument about white dwarfs between Eddington and Chandrasekhar is given, the inspiration we draw from the argument and the style of Chandrasekhar' s research are discussed.
3、However, Chandrasekhar showed that for a sufficiently massive star the gravitational collapse continues until the star shrinks to a point.