eddington 中文意思是什麼
eddington
解釋
n. 名詞 埃丁頓〈姓氏〉。-
Emission below the eddington limit would have been fairly straightforward to explain
這場爆炸的強度要是低於艾丁頓上限的話，解釋起來就簡單了。 -
His arguments were opposed by arthur eddington, who believed that something would inevitably stop the collapse
他的觀點遭到亞瑟?埃丁頓反對，他相信某些東西會不可避免阻止坍塌。 -
In 1919, sir arthur eddington tested this prediction during a solar eclipse by measuring starlight bending around the sun
1919年，阿瑟?艾丁頓通過在日全食時測量太陽邊緣處的星光對這個預言進行了驗證。 -
X - ray flashes had previously been detected from some neutron stars, but they never exceeded the eddington limit by very much
以往天文學家就曾觀測到過從中子星發出來的x射線閃光，但其亮度從來不會超過艾丁頓上限太多。 -
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:對幾種常用的二流近似， issaacs二流近似， eddington近似， c - c二流近似以及-二流近似和- eddington近似都作了介紹，然後我們利用二流近似對反射率進行計算求解。 -
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
本文採用與觀測結果具有相同形式的球狀星團空間密度分佈函數，在給定兩種球狀星團系統的初始質量譜（冪律的和對數高斯的）和兩種球狀星團系統的初始速度分佈函數（愛丁頓速度分佈函數和常數的速度彌散度）條件下，我們採用montecarlo的方法對球狀星團系統的動力學演化進行討論。
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