From the Large Magellanic Cloud or LMC, their origin is explained by the decay of binary systems.

从麦云（LMC）来看，它们的起源可以用双系统的衰变来解释。

And if the computer simulation is correct, not only many hypervelocity stars, but also neutron stars as well as black holes are rushing towards our galaxy from the Large Magellanic Cloud.

如果计拟是正确的，不仅有许多超高速恒，还有中子和黑洞从麦云冲向我们的系。

This massive star called HH 1177 is in a galaxy called Large Magellanic Cloud.

这颗名为HH 1177的质量恒位于麦云中。

Both are irregular in shape, though the Large Magellanic Cloud is barely coherent enough to qualify as a disrupted, though small, barred spiral.

这两者的形状都是不规则的，尽管麦云几乎没有足够的连贯性，以称得上是一个中断的，但小的棒旋系。

It was discovered in the Tarantula Nebula, a huge gas cloud in the Large Magellanic Cloud galaxy.

它是在狼蛛云中发现的，这是麦系中的一个巨的气体云。

The images are in galaxies beyond the Large Magellanic Cloud and Small Magellanic Cloud.

这些图像属于麦系和小麦系之外的系。

Maybe the Large Magellanic Cloud orbiting the Milky Way.

也许是围绕银河系运行的麦云。

If you look up at the southern sky, you can actually see two of these small galaxies, the largest of the small galaxies that are orbiting our Milky Way, the Large Magellanic Cloud and the Small Magellanic Cloud.

如果你抬头看向南方的天空，实际上可以看到两个这样的小系， 它们是绕着我们银河系运行的小系中最的两个，麦云和小麦云。

And she was astute enough to notice, you know, not only were these stars varying that she was finding in the large Magellanic Cloud and the small Magellanic Cloud, but there was this correlation.

她足够敏锐地注意到，不仅她在麦云和小麦云中发现这些变，而且它们之间存在着这种关联。

These two dwarf galaxies are the Magellanic clouds which, together with at least 80 others, make up what's known as the local group of galaxies.

这两个矮系是麦云，它与至少 80 个其他系一起，构成了所谓的本系群。

The Magellanic clouds have a stellar mass of the order of a billion solar masses, and the Milky Way, a hundred billion solar masses.

麦云的恒质量约为数十亿个太阳质量，而银河系则有数百亿个太阳质量。

The Cepheid variable stars that Leavitt studied are in the Magellanic clouds, known today to be galaxies outside the Milky Way.

勒维特研究的造父变位于麦云中，如今已知这些云是银河系外的系。

Star-forming regions, one is in the Milky way, our galaxy and two nearby galaxies, the Magellanic clouds.

恒形成区，一个是在银河系，我们的银河系和附近的两个系，麦云。

Our large Magellanic Cloud, our nearest galactic neighbor, is orange instead of its more familiar blue-white.

我们的麦云，作为最近的银河系邻居，呈现出橙色而非更为人熟知的蓝白色。

This is the Large Magellanic Cloud.

这是麦云。

The large Magellanic cloud is about 160,000 light-years away.

麦云距离地球约16万光年。

Some of these, you may have seen when observing the night sky, or you may have heard of, like the Large Magellanic Cloud and the Small Magellanic Cloud.

其中一些，你可能在观察夜空时见过，或者你可能听说过， 比如麦云和小麦云。

The Tarantula Nebula is located in the Large Magellanic Cloud at a distance of about 150,000 light-years.

蜘蛛云位于麦云中，距离我们约 15 万光年。

And the third region that we want to study is called NGC346, is farther away still about 200,000 light-years in the Small Magellanic Cloud, yet another galaxy.

我们要研究的第三个区域称为 NGC346，距离麦系约 200,000 光年，是另一个系。

A specific task that Levitt took on was to examine some of the photographic plates of stars in the Small Magellanic Cloud, SMC, and the Large Magellanic Cloud, LMC.

莱维特承担的一项具体任务是检查一些小麦云（SMC）和麦云（LMC）中恒的照相板。