neutron stars

  • Web中子星

Web Definition

1.
中子星
如果连恒星演化的最后阶段也算在内，最小的星大概是中子星 (neutron stars)，中子星是大质量恒星在临终爆炸后的一种遗物， …
forum.hkas.org.hk|Based on 85 pages

Sample Sentence

Definition:
AllAll,中子星中子星
Category:AllAll,OralOral,WrittenWritten,TitleTitle,TechnicalTechnical
Source:AllAll,DictionaryDictionary,WebWeb
Difficulty:AllAll,EasyEasy,MiddleMiddle,HardHard
1.
One of the best possible sources for gravitational waves would be a merger between compact binary neutron stars.
观测引力波的最佳时机之一就是两颗中子星互相吞噬的过程。
guān cè yǐn lì bō de zuì jiā shí jī zhī yī jiù shì liǎng kē zhōng zǐ xīng hù xiāng tūn shì de guò chéng 。
article.yeeyan.org
2.
A third topic is that of the high-density colour superconductive state of matter, which may be present in the core of neutron stars.
第三个议题是，在高密度色超导物质的状态，这可能是在中子星的核心存在。
dì sān gè yì tí shì , zài gāo mì dù sè chāo dǎo wù zhì de zhuàng tài , zhè kě néng shì zài zhōng zǐ xīng de hé xīn cún zài 。
www.ccebook.net
3.
He said the neutron stars can be no larger than about 20. 5 miles (33 kilometers) across.
他指出，这些中子星的直径不可能超过20.5英里（33公里）。
tā zhǐ chū , zhè xiē zhōng zǐ xīng de zhí jìng bù kě néng chāo guò èr shí diǎn wǔ yīng lǐ ( sān shí sān gōng lǐ ) 。
huzhangao.blog.163.com
4.
To find out how strong the crusts of neutron stars really are, Horowitz and a colleague created a computer simulation of a star's surface.
为了发现中子星的地壳到底有多么硬，Horowitz和一位同事建立了一颗星球表面的计算机模拟程序。
wèi le fā xiàn zhōng zǐ xīng de dì qiào dào dǐ yǒu duō me yìng , Horowitz hé yī wèi tóng shì jiàn lì le yī kē xīng qiú biǎo miàn de jì suàn jī mó nǐ chéng xù 。
bbs.chinadaily.com.cn
5.
Strong gravitational waves are thought to be produced by the collision of two neutron stars.
在两颗中子星星体之间的作用被认为会产生很强的重力波动。
zài liǎng kē zhōng zǐ xīng xīng tǐ zhī jiān de zuò yòng bèi rèn wéi huì chǎn shēng hěn qiáng de zhòng lì bō dòng 。
www.ecocn.org
6.
One of the neutron stars is a pulsar; it emits radio pulses at regular intervals as it spins 45 times per second.
其中一颗为脉冲星，该脉冲星以每秒45周的旋频率向宇宙中发射有规律的无线电波。
qí zhōng yī kē wèi mài chōng xīng , gāi mài chōng xīng yǐ měi miǎo sì shí wǔ zhōu de xuàn pín lǜ xiàng yǔ zhòu zhōng fā shè yǒu guī lǜ de wú xiàn diàn bō 。
www.astronomy.com.cn
7.
however , it is now proposed that the conversion of neutron stars to strange stars is another possible origin of gamma - ray bursts.
不过，近期有研究指出，伽玛射线爆发现象，也可能是由一颗中子星转变为奇异星时所产生的。
bú guò , jìn qī yǒu yán jiū zhǐ chū , jiā mǎ shè xiàn bào fā xiàn xiàng , yě kě néng shì yóu yī kē zhōng zǐ xīng zhuǎn biàn wéi qí yì xīng shí suǒ chǎn shēng de 。
www.ichacha.net
8.
Due to the existence of high viscosity in strange matter, strange stars can reach much shorter period than neutron stars.
由于奇异星有很高的粘度，它的自转周期会比中子星短得多。
yóu yú qí yì xīng yǒu hěn gāo de nián dù , tā de zì zhuàn zhōu qī huì bǐ zhōng zǐ xīng duǎn de duō 。
www.lcsd.gov.hk
9.
The most likely explanation for GRB050709 is that it was produced by a collision of two neutron stars, or a neutron star and a black hole.
对于GRB050709，最可能的解释认为，它是两颗中子星，或者一颗中子星和一个黑洞碰撞的结果。
duì yú GRB líng wǔ líng qī líng jiǔ , zuì kě néng de jiě shì rèn wéi , tā shì liǎng kē zhōng zǐ xīng , huò zhě yī kē zhōng zǐ xīng hé yī gè hēi dòng pèng zhuàng de jié guǒ 。
article.yeeyan.org
10.
For M15, the HST astronomers relied on an earlier estimate of the number of neutron stars in the cluster.
对于M15，哈勃空间望远镜的结论建立在早期对其中中子星数量的估计之上。
duì yú M shí wǔ , hā bó kōng jiān wàng yuǎn jìng de jié lùn jiàn lì zài zǎo qī duì qí zhōng zhōng zǐ xīng shù liàng de gū jì zhī shàng 。
bbs.astron.ac.cn