在 中文 中使用 白矮星 的示例及其翻译为 英语
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然而，一些白矮星，范围从1%到4%，显示出红外辐射，表明它们被尘埃盘或环包围。
However, in 1 to 4% of cases, white dwarfs have shown infrared emissions that indicate that they are surrounded by dust disks or rings.当它到达临界质量（约合1.4倍太阳质量）时，白矮星坍缩并发生爆炸。
When it reaches a critical mass(about 1.4 times the mass of the Sun), the white dwarf collapses and explodes.结果是，至少根据他们的计算，这些白矮星可以在类似___的爆炸中重新点燃，产生更重的元素。
It turns out that, at least according to their calculations, these white dwarfs could reignite in a supernova-like explosion, generating heavier elements.我严重相信新天堂将包括新的星系,行星,卫星,白矮星,中子星,黑洞,和类星体吗?
Do I seriously believe the new heavens will include new galaxies, planets, moons, white dwarf stars, neutron stars, black holes, and quasars?白矮星是一种小而密集的恒星，它们烧掉了大部分的氢和氦气体。
White dwarfs are the small, dense remnants of stars that have burnt off most of their hydrogen and helium fuel.因此，在巨大的分支阶段，YORP效应非常重要，但是在恒星变成白矮星之后几乎不存在。
Hence, the YORP effect is very important during the giant branch phase, but almost non-existent after the star has become a white dwarf.”.这很有趣，也不同于科学家们的预期--白矮星与其他恒星相撞会变成1a型超新星。
This is interesting and different from what scientists expect- that white dwarfs colliding with other stars should turn into type 1a supernovae.Em巴西大学和研究机构的一群天文学家观察到，由于伴侣的缘故，一颗星降为白矮星状态。
A group of astronomers in Brazilian universities and research institutions observed a star demoted to white dwarf status because of companion.因此，它们的恒星组成成份也是类似的，都含有红巨星（M44中至少有5颗）和一些白矮星。
Consequently, also the stellar populations are similar, both containing red giants(M44 at least 5 of them) and some white dwarfs.他说，白矮星模型有太多的问题，最主要的一个是无法解释为什么一些AXP与超新星遗迹有联系。
The white-dwarf model has many problems, he says, the chief one being that it cannot explain why some AXPs are associated with young supernova remnants.白矮星如果有邻近的伴星，则可能成为Ia超新星。
White dwarf stars, if they have a near companion, may then become Type La supernovae.另一种假设是，它是由白矮星死亡时喷出的气体形成，这使它成为第二代行星。
Another hypothesis is that it formed out 然后气体落在白矮星上，沿着磁带与磁星相遇的皮带产生X射线。
同时，更加精确的白矮星内部化学组分也可以作为“宇宙学计时器”来确定银河系的星族年龄。
A precise knowledge 我们需要等到恒星变成白矮星时才知道碎片在哪里，以了解圆盘是如何形成的。
We need to know where the debris is by the time the star becomes a white dwarf to understand how discs are formed.气体在白矮星周围堆积，最终变得足够稠密，足以在核聚变爆炸中点燃。
Gas piles up around the white dwarf and ultimately becomes dense enough to ignite in a burst of nuclear fusion.UCLA团队研究的白矮星距离地球200―665光年之间。
The white dwarf star studied by the UCLA team is between 200 and 665 light years from Earth.最新发现表明，当前关于白矮星形成和恒星之间相互作用的理论中缺少某些东西。
The latest finding suggests that something is missing in the current theory on the formation of white dwarfs and the interaction between stars.另一种假设认为，它由白矮星死亡过程中喷射的气体形成，是第二代行星。
Another hypothesis is that it formed out 当一对白矮星合并时，研究人员预计会发生1a型超新星，或大型恒星爆炸。
When pairs of white dwarfs coalesce, researchers expect something called a type 1a supernova, or large stellar explosion to occur.
