We can see nearby galaxies, like the Andromeda Galaxy, that are interacting with the Milky Way Galaxy.

我们可以看到附近的星系，比如仙女座星系，它们与银河系相互作用。

Today's astrophysics question: Does the spin of a galaxy influence the spin of other nearby galaxies?

星系的自旋是否会影响附近其他星系的自旋？

The Large Cloud sports the biggest and most active star forming gas cloud in any nearby galaxy: the Tarantula Nebula.

大麦哲伦星云促成了附近星系中最大、最活跃的气体云：狼蛛星云。

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

恒星形成区，一个是在银河系，我们的银河系和附近的两个星系，麦哲伦星云。

One is in the Milky Way, our galaxy and two are in nearby galaxies, the Magellanic Clouds.

一个在银河系， 我们的星系， 两个在附近的星系，即麦哲伦星云。

When the gases and dust of nearby galaxies get pulled into the event horizon, the atoms gain energy and heat up.

当附近星系的气体和尘埃被拉入事件视界时，原子获得能量并升温。

Now, the fact is that nearby galaxies might be going away from us or toward us, based on how they’re moving within their local cluster.

现在，事实是附近的星系可能会远离我们或靠近我们，这取决于它们在本地星团中的移动方式。

Now, the fact is that nearby galaxies might be going away from us or toward us, based on how they're moving within their local cluster.

现在，事实是附近的星系可能 会远离我们或接近我们，这 取决于它们在本地星团内的移动方式。

The main goal is to understand what is the difference in the way in which stars form in our own galaxy, and also nearby galaxies.

主要目标是了解恒星在我们自己的星系和附近星系中形成的方式有何不同。

The last supernova that sent detectable neutrinos to Earth was in 1987 on the edge of the Tarantula Nebula in the large Magellanic Cloud, a nearby galaxy.

最后一次向地球发送可探测中微子的超新星发生在 1987 年，位于附近星系大麦哲伦星云中的狼蛛星云边缘。

That meant GRBs were either VERY nearby — no more than a few hundred light years — or that they were coming from INCREDIBLY far away, so far that even nearby galaxies weren't affecting the distribution!

这意味着 GRB 要么非常近——不超过几百光年——要么就来自非常遥远的地方，远到连附近的星系都不会影响到它的分布！