内德的儿子当时正在用望远镜观看银河星团。
所有的三项发现都指出，在宇宙最大的稳定结构，即星系和巨大银河星团中有动态的运动。
All three findings pointed to dynamic movement in galaxies and in monstrous galactic clusters, the largest stable structures in the universe.
我们可以观测到，球状星团在银河系周围的巨大光晕中广泛分布。
Globularclusters can be found spread largely in a vast halo around our galaxy.
因此，研究球状星团可以向我们揭示银河系的历史。
Studyingglobular clusters therefore tells us about the history of our galaxy.
相反的，他们只能局限于直接测量轨道上的物体：银河系中的气体，恒星，以及较远的卫星星系和星团。
Instead they are limited to directly measuring objects in orbit: the galaxy's gas and stars, as well as distant satellite galaxies and star clusters.
因此，研究球状星团可以向我们揭示银河系的历史。
Studying globular clusters therefore tells us about the history of our galaxy.
回到过去，回到我们的星系刚形成时，可能有数千球状星团在银河系内游荡。
Back in the old days, back when our Galaxy first formed, perhaps thousands of globular clusters roamed our Galaxy.
但是即使是这个定义，也缺失了许多天文学家认为非常重要的特性，比如支配当地的环境，银河系就是这样支配周围的球状星团的。
But even this misses out various characteristics that astronomers think are important, such as dominating the local environment, in the way the Milky way dominates the globular clusters nearby.
图中的蓝色斑点是银河系的恒星，背景中的蓝白色暮霭是来自更古老的恒星星团的光。
The blue specks are Milky Way stars, and the bluish-white haze in the background is light from older star clusters.
球状星团曾经统治着银河系。
我们可以观测到，球状星团在银河系周围的巨大光晕中广泛分布。
Globular clusters can be found spread largely in a vast halo around our galaxy.
半人马座是已知的漫游在我们银河系光环中的200多个星团中最大的。
Omega Cen is the largest of 200 or so known globular clusters that roam the halo of our Milky Way galaxy.
在遥远的背景天空中的是我们银河系的光带、昴星团，以及仙女座星云。
Visible in the distant background sky is the band of our Milky Way galaxy, the Pleiades open clusters of stars, and the Andromeda galaxy.
上千球状星团围绕着银河，其中包含一些宇宙中最老的星星。
Surrounding the Milky Way are thousands of spherical globular star clusters containing some of the oldest stars in the Universe.
小麦哲伦云的左边，明亮的白色物体，是银河系内一个球状星团，被称作杜鹃47。
The bright white object just to the left of the SMC is a globular cluster of stars in the Milky Way known as 47 Tucana.
NGC2818是银河系中少数几个位于疏散星团内部的行星状星云之一。
NGC 2818 is one of very few planetary nebulae in our galaxy located within an open cluster.
2008年，科学家们就报告说他们发现了上百个银河系星团正在以每小时220万英里(360万公里)的速度的朝着同一方向移动。
In 2008 scientists had reported the discovery of hundreds of galaxy clusters streaming in the same direction at more than 2.2 million miles (3.6 million kilometers) an hour.
天文学家们已经用多种望远镜扫描了整个天空，探测到了银河系内和球状星团附近的脉冲星。
Astronomers have scanned the complete sky with various telescopes and detected pulsars in the Milky Way and nearby globular clusters.
拱门星团是我们的星系中最密集的恒星群，它位于银河系拥挤的中心区。
The Arches is the densest star cluster in our Milky Way galaxy and resides in our galaxy's crowded core.
疏散星团动力学及形成过程的研究对于恒星动力学理论和银河系恒星形成理论具有重要意义。
Studies of the dynamics and formation process of open clusters are of great significance for stellar dynamics and star formation in the Galaxy.
在我们的银河系里，大约有200个球状星团拥有宇宙中一些最古老的星球，不过，却一直没有发现年轻星球的踪影。
The roughly 200 globular clusters in our Milky Way galaxy contain some of the oldest known stars in the universe; young inhabitants are nowhere to be seen.
右上方明亮的微红色天体是银河系的中心，距离星团100光年。
The bright reddish object at upper right is the center of our galaxy, residing 100 light-years away from the Arches cluster.
本模型以银河系球状星团的形成和演化为出发点，但同样普适于其它星系中球状星团的形成和演化。
It is shown as well that this model is successful to apply not only to GCs in our Galaxy, but also to those in other galaxies as they have a universal formation process.
球状星团与疏散星团年龄相比要老得多，表明它们是在银河系形成初期形成的恒星系统。
It also shows that all globular clusters in our Galaxy are very old, much older than the oldest open clusters in the Galactic disk.
宇宙里动人心弦的影像，涵盖了错综复杂的尘埃带、明亮的星云星团，分散在我们银河中心星场。
The breathtaking cosmic vista shows off intricate dust lanes, bright nebulae, and star clusters scattered through our galaxy's rich central starfields.
宇宙里动人心弦的影像，涵盖了错综复杂的尘埃带、明亮的星云星团，分散在我们银河中心星场。
The breathtaking cosmic vista shows off intricate dust lanes, bright nebulae, and star clusters scattered through our galaxy's rich central starfields.
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