1.
A typical globular cluster has about 1 million stars.
一个典型的球状星团包含1百万恒星。
2.
Study on Binary Stellar Populations of Globular Clusters in M31
M31中球状星团的双星族合成研究
3.
Smaller groups of stars called globular clusters often surround spiral galaxies.
称作球状星团的小型恒星团体经常环绕在旋涡星系周围。
4.
How could we be sure that these globularlike clusters really were younger versions of the globulars in our own galaxy?
我们如何能确定这些类球状星团就是我们星系里球状星团当年的样子呢？
5.
The old age typical of the globular clusters in our galaxy has had a profound impact on the study of globulars in general.
在我们星系中，这些典型的老年球状星团对于一般球状星团的研究影响深远。
6.
The discovery of young and intermediate-age globular clusters opens up a whole new way to study how globulars form.
年轻及中年球状星团的发现，为球状星团的形成开启了新的研究道路。
7.
What is it about globulars that overcomes these odds?
能克服上述不利情况的球状星团，有何特异之处？
8.
For this purpose the study of globular clusters is most instructive.
在这个问题上球状星团的研究最富有指导意义。
9.
Maybe globulars go on forming whenever conditions permit.
也许在条件适当时，球状星团便会不断地形成。
10.
The Absolute Proper Motion of M3 and Its Orbit in the Galaxy;
球状星团M3的绝对自行测定及其轨道计算
11.
Recently astronomers have discovered these intermediateage globular clusters in several elliptical galaxies.
最近，天文学家已在数个椭圆星系里发现了这类中龄的球状星团。
12.
This finding corroborates the link between the merger process and the formation of globulars.
这项发现确认了星系融合过程与球状星团形成之间的关联。
13.
There is no absolutely sharp cutoff distinguishing galaxies from globular clusters.
在星系和球状星团之间没有任何不可逾越的鸿沟。
14.
Calculation for the Density Distribution of the Star Numbers near to the Magnetic Black??Hole in the Globular Custer
球状星团中荷磁黑洞附近星的投影密度分布的计算
15.
It dawned on astronomers that the crowded conditions in globulars could be the deciding factor.
天文学家渐渐明白：球状星团内的拥挤状态可能是决定因素。
16.
Globular cluster is a group of tens of thousands to millions of stars bounded under gravity.
球状星团由上万至百万的恒星组成，在一个细小範围内由万有引力维系的集团。
17.
A study of many globular clusters gives another important bit of information.
对许多球状星团进行研究之后，使我们得到一些重要信息。
18.
Space Distribution, Motional Orbits and Monte Carlo Simulation of Globular Clusters in the Galaxy;
银河系中球状星团的空间分布、运动轨道及Monte Carlo模拟