Emission below the eddington limit would have been fairly straightforward to explain 这场爆炸的强度要是低于艾丁顿上限的话，解释起来就简单了。
2.
His arguments were opposed by arthur eddington , who believed that something would inevitably stop the collapse 他的观点遭到亚瑟?埃丁顿反对，他相信某些东西会不可避免阻止坍塌。
3.
In 1919 , sir arthur eddington tested this prediction during a solar eclipse by measuring starlight bending around the sun 1919年，阿瑟?艾丁顿通过在日全食时测量太阳边缘处的星光对这个预言进行了验证。
4.
X - ray flashes had previously been detected from some neutron stars , but they never exceeded the eddington limit by very much 以往天文学家就曾观测到过从中子星发出来的x射线闪光，但其亮度从来不会超过艾丁顿上限太多。
5.
Second is reflectivity : issaacs double - streams approximating , eddington approximating , c - c double - streams approximating , - double - streams approximating and - eddington approximating is explained and used to calculate the reflectivity . at last , the two parameters is used in the above model to obtain the result 其次是反射率:对几种常用的二流近似, issaacs二流近似, eddington近似, c - c二流近似以及-二流近似和- eddington近似都作了介绍,然后我们利用二流近似对反射率进行计算求解。
6.
Given the initial conditions including ( 1 ) number density distribution in space which has the similar form to the present day ones , ( 2 ) both the power law and gaussian mass functions for clusters , and ( 3 ) two different velocity distributions which one has a constant dispersion and the other is described by the eddington formula , the dynamical evolution of globular clusters in our milky way galaxy is investigated in detail by means of monte carlo simulations 本文采用与观测结果具有相同形式的球状星团空间密度分布函数，在给定两种球状星团系统的初始质量谱(幂律的和对数高斯的)和两种球状星团系统的初始速度分布函数(爱丁顿速度分布函数和常数的速度弥散度)条件下，我们采用montecarlo的方法对球状星团系统的动力学演化进行讨论。
