Chandrasekhar信息详情
n.（Chandrasekhar）人名；（印、英）钱德拉塞卡尔
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。
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。
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。
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。
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。
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。
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
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.
However, Chandrasekhar showed that for a sufficiently massive star the gravitational collapse continues until the star shrinks to a point.
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.