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These events include two kinds of stellar explosions:(1) nova explosions, in which one of the two members of a binary star system hurls dust and gas into space;(2) much more violent supernova explosions, in which a star collapses, then throws off most of its matter.

这些事件包括两种类型的恒星爆发:(1)新星爆发,双星系统中的一员将气体和尘埃猛烈抛入太空;(2)更为猛烈的超新星爆发,那是一颗恒星崩溃时几乎把它所有物质都抛出去了。

The observation confirmed a decade of speculation that a warp in the young star's dust disk may actually be a second disk inclined to the star.

这项观测确定了10年来的推测学说,即年轻恒星的尘埃盘可能实际上时第二个尘埃盘向恒星一侧倾斜。

Imagine a planet-forming disk surrounding such a star: The disk, like the star itself, would be rich in heavy elements.

想象一个形成行星的磁盘周边这样一个明星:磁盘一样,明星本身,将丰富的重元素。

Imagine a planet-forming disk surrounding such a star: The disk, like the star itself, would be rich in heavy elements.

想像一个形成行星的磁盘周边这样一个明星:磁盘一样,明星本身,将丰富的重元素。

Highly energetic X-rays are also detected from the young star, partially absorbed by streams of material flowing from the disk onto the star.

年轻恒星的高能x射线同样被探测到,部分通过从圆盘到恒星的物质流吸收。

On the formation mechanism of brown dwarfs astronomers have different opinions, the more common projectile theory, the former star's light caused by erosion of the nuclear theory of opacity constraints of splitting theory, the original star's disk instability theory.

关于褐矮星形成的机制天文学家们众说纷纭,比较常见的有抛射理论、前恒星核的光致侵蚀理论、不透明度制约的分裂理论、原恒星盘的不稳定性理论等。

As streams of material spiral from the disk onto the star, its mass increases and it brightens and heats up dramatically. The resulting outburst causes temperatures to rise in the star's surrounding disk.

随着物质流从行星盘落向中央恒星,恒星的质量增加并剧烈的变热(重力势能转化为热能——译注),结果产生的爆发导致周围的行星盘变热。

The telescope showed that a previously detected planet around the nearby star Epsilon Eridani is orbiting at a 30-degree angle to our line of sight, the same inclination as the star's dust disk.

哈勃望远镜显示一颗曾经被我们观测到的轨道与我们的视线成30度角,位于Epsilon Eridani附近的行星,与恒星的尘埃盘有相同的倾角。

The centrifugal force from that prevents some of the gas from reaching the forming star. Instead, it forms an "accretion disk" around the star. The disk radiates away its energy and cools off.

而离心力阻止一些气体到达正在形成的恒星,相反,他们在恒星周围形成一个&吸积盘&,它向外辐射能量并冷却。

Firstly, we adopt the same parametersthat well fit the Milky Way disk to the M31 disk evolution. We found thatthe obtained gas surface density and star formation rate profiles do notfit the M31's observation. This demonstrates that the star formation history inthe M31 disk may totally different from that in the Milky Way disk.

首先,我们将银河系的化学演化模型应用于M31上,发现银河系的恒星形成速率与气体面密度的关系并不符合M31的观测特征,这说明两者拥有不同的恒星形成历史。

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