neutron star
美 
英
- na.【天】中子星
- 網絡成中子星；脈沖星中子星；中子星座
英漢解釋
英英解釋
例句
In the nebula's very center lies a pulsar: a neutron star as massive as the Sun but with only the size of a small town.
在星云的正中心有一個脈沖星：一個中心星，它擁有和太陽類似的質量而只有一個小村莊那么大。
(Kusenko likens it to "a bullet passing through a cloud of vapor. " ) And if it runs into a neutron star?
（Kusenko把這比作“一顆子彈穿過一層蒸汽”）那么它跑進中子星會發生什么呢？
Badenes's team examined archival observations and found a white dwarf and neutron star orbiting one another extremely closely.
Badenes的團隊試驗檔案觀測并發現白色小的中子星體非常近的圍繞另一個運轉。
And this really changed our whole concept of astronomy, the existence of these neutron star binaries.
對于天文學的概念，這些中子雙星的，存在，現在一部分是。
And I take a little bit of matter m, and I drop it from a large distance onto the neutron star.
從很遠的距離扔到，中子星上，那個小物體。
Astarquake is thought to be the tearing apart of the surface of a neutron star, much like an earthquake here on Earth.
恒星地震拒信可以撕裂中子星表面，其所能產生的破壞力很像地球上的地震。
It was the first time that astronomers have measured the rate of cooling of a young neutron star.
這是天文學家第一次測量到了年輕中子星的冷卻速率。
However, you will never see pulsations, because a black hole has no surface, like a neutron star.
你將不會看到脈動，因為黑洞沒有表面，它不像中子星，不存在兩個熱點可以。
Now, two teams of physicists say they have more direct evidence for superfluidity in the heart of a neutron star.
現在，兩個小組的物理學家宣稱他們掌握了中子星核心中超流的更直接的證據。
A ten-gram object thrown onto a neutron star-- the reason being that this velocity becomes enormously high.
原因就在于-，速度，變得無窮大，若扔到中子星的物體。
and ensuing explosion would blow off the outer envelope of the star and leave behind the core as a neutron star.
按此模型，引起的突然壓縮和隨后的爆發會把恒量的外部包層吹跑，留下的核成為一顆中子星。
Smolin's predictions, including ideas about cosmological inflation and the mass of the heaviest stable neutron star, have held up so far.
Smolin的預測，包括宇宙暴脹學說和最重穩定中子星的質量都有待驗證。
After the supernova, the leftover matter could either have collapsed into a black hole or an extremely dense neutron star.
超新星爆發以后，剩余的物質可能塌縮為一個黑洞，也可能形成一顆密度極大的中子星。
In theory, the first step toward producing a millisecond pulsar is the formation of a neutron star when a massive star goes supernova.
理論上，形成一顆毫秒脈沖星的第一步，是一個大質量恒星在成為超新星而爆發后留下的中子星。
It might therefore seem like an easy task to create a 'neutron star' at home.
因而看來在家里制造一個“中子星”也似乎是一個簡單的活。
If the neutron star is too large, the gravitational forces overwhelm the pressure gradients and collapse cannot be halted.
如果中子星太大，吸引力勝過氣壓梯度，塌陷便不能被阻止。
At this point, a neutron star pair, or even a neutron star-black hole pair, is formed.
此刻，一個雙中子星、甚至中子星-黑洞對將形成。
This seemingly gentle structure also harbors a very powerful spinning neutron star that may be the central remnant from the initial blast.
這些外表柔和的結構也蘊藏著一個很強大的旋轉的中子星，那可能是來自最初爆炸的灰燼的中心。
Three years later, Salla's nav computer malfunctioned and deposited her vessel on a collision course with a neutron star.
三年后，薩拉的飛船因導航電腦故障，鎖定航線向一顆中子星撞去。
And you don't really ; have to be infinitely far away; you just have to be much further away than the radius of the neutron star.
從無窮遠處來，你只要在遠大于；，中子星半徑的地方，當物體撞到。
The model comprising accretion onto a neutron star or black hole companion must still be considered a favored hypothesis.
在中子星或黑洞伴星上發生吸積的模型，仍應看成是一個有價值的假說。
The only things more dense are black holes, as a teaspoonful of neutron star matter would weigh about 100 million tons.
比它密度再大的就只有黑洞了，只需要一勺匙中子星的質量就可以達到100萬噸。
Basically, a black hole is formed when a very, very large star has a supernova event which can result in a neutron star or a black hole.
基本上，黑洞都脫胎于恒星，如果這顆恒星爆發成一顆非常，非常碩大的超新星，那么就可能會產生中子星或黑洞。
Since a 7-solar-mass is too large to be a white dwarf or neutron star, it must be a black hole.
因為有著7個太陽質量的星體不可能是白矮星或中于星，所以它一定是黑洞。
Such "pulsar glitches" likely result from brief interactions between the neutron star's solid crust and superfluid interior.
這種“脈沖星故障”很可能源于中子星堅硬的地殼與超流內部的短暫作用。
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.
對于GRB050709，最可能的解釋認為，它是兩顆中子星，或者一顆中子星和一個黑洞碰撞的結果。
The other neutron star does not beam radio pulses toward Earth, so it remains unseen except for its gravitational influence.
另外一顆中子星沒有發出朝向地球的脈沖信號，所以除了重力影響，它不能被觀測到。
Properties of nuclear matter and neutron star are described in relativistic mean field theory with density-dependent effective interactions.
基于密度相關有效相互作用的相對論平均場理論，研究了核物質和中子星的性質。
In this case, you have to open and close it with exactly the same frequency as the rotation of the neutron star.
在這個例子里，你必須以和中子星，旋轉相同的頻率，對其進行開關。
The model comprising accretion onto a neutron star or black hole companion must still be considered a favored hypothesis.
在中子星或黑洞伴星上發生吸積的模型，仍應看成是一個有價值的假說。
The explosion could also cause a neutron star or result in the formation of a black hole 1300 light years from Earth, reports news. com. au.
au的報道稱，爆炸還會形成一個中子星（neutronstar），或者是一個距地球1300光年的黑洞。
These binary systems consist of a neutron star orbiting around a supergiant star.
這些雙星系統由一個巨星和圍繞其的中子星組成。
Each star of the closely-packed system is a dense neutron star, spinning extremely fast, radiating X-rays in pulses .
這個緊密系統的每一顆星都是致密的中子星，自旋非常快，輻射著X射線脈沖。
Frequent Space Museum visitors should know that neutron star is one of the possible final products of stellar evolution.
經常參觀太空館的人該知道，中子星是恒星演化至末期的結果之一。
Now, two teams say they have direct evidence of such bizarre "superfluidity" in a neutron star, and other researchers seem convinced.
現在，兩個小組宣稱他們掌握了這種中子星內奇異超流體的直接證據，并且其他研究者似乎相信這一發現。
A millisecond pulsar is a super compact neutron star, whose spin is highly accelerated by mass transferred from a companion star.
毫秒脈沖星是密度極大的中子星，其旋轉被從伴星轉移來的的物質大大地加快了。
When the neutron star moves behind the donor star, all the x-rays are absorbed by the donor star and you get x-ray eclipses.
后面移動，所有的x射線都會被，供體星吸收，得到x射線食，換句話說。
''This neutron star was born so hot that nuclear fusion happened on its surface, producing a carbon atmosphere just 10 centimetres thick. ''
“這顆中子星產生時溫度如此之高，其表面還在進行核子融合，從而產生了只有10厘米厚的碳大氣層。”
As a black hole or neutron star destroys a star, tremendous amounts of radiation are released.
當黑洞或中子星將一顆恒星毀滅時將會產生巨大的輻射。
At what distance from the neutron star's surface is the radiation created that the radio observatories detect?
我們觀測到的射電信號是在離中子星表面多遠的距離上生成的？
A supernova can leave behind a dense, rapidly spinning core made almost completely of neutrons , called a neutron star.
超新星爆發后可能會留下一個極高密度、快速旋轉的、幾乎完全由中子構成的核心，即中子星。
