neutron stars的意思

neutron stars中文翻譯：

n.[天]中子星

相似詞語短語

stars───v.點綴；成輻射狀開裂；使擔任主角（star的第三人稱單數）；abbr.specializedtrainingandreassignmentstudents經過專門訓練后再分配的學生；stationaryautomotiveroadstimulator(Toyota)汽車公路固定刺激物（豐田汽車）；n.明星類，明星（star的復數形式）

neutron star───n.[天]中子星；n.中子星

fallen stars───隕星

try stars───試試星星

dark stars───[天]暗星

famous stars───著名明星

dying stars───垂死的星星

zero stars───零星

party stars───派對明星

雙語使用場景

Neutron stars are, after all, a little less extreme than black holes, Big Bangs and supernovae...───畢竟中子星并沒有黑洞、大爆炸、超新星等等那么極端。

So instead of looking at many neutron stars, researchers needed to look at only this one.───因此，不同于以往觀察許多中子星，研究人員們只需要觀測這一個中子星即可。

Neutron stars are created when massive stars run out of fuel and collapse.───中子星是在大型恒星耗盡燃料后崩潰而產生的。

One of the best possible sources for gravitational waves would be a merger between compact binary neutron stars.───觀測引力波的最佳時機之一就是兩顆中子星互相吞噬的過程。

A third topic is that of the high-density colour superconductive state of matter, which may be present in the core of neutron stars.───第三個議題是，在高密度色超導物質的狀態，這可能是在中子星的核心存在。

He said the neutron stars can be no larger than about 20. 5 miles (33 kilometers) across.───他指出，這些中子星的直徑不可能超過20.5英里（33公里）。

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.───為了發現中子星的地殼到底有多么硬，Horowitz和一位同事建立了一顆星球表面的計算機模擬程序。

Strong gravitational waves are thought to be produced by the collision of two neutron stars.───在兩顆中子星星體之間的作用被認為會產生很強的重力波動。

One of the neutron stars is a pulsar; it emits radio pulses at regular intervals as it spins 45 times per second.───其中一顆為脈沖星，該脈沖星以每秒45周的旋頻率向宇宙中發射有規律的無線電波。

英語使用場景

Though the maximum masses and corresponding radii are similar, bare strange quark stars and normal neutron stars could be distinguished in the regime of low masses.

Before the two neutron stars collide, they would orbit each other as a binary system.

Neutron stars are the second exhibit in the gallery of stellar corpses.

Pulsars, neutron stars and quark stars are then created based on their mass.

Moreover, because of their intense density, neutron stars exert strong gravitational force on their binary companion.

They were therefore called neutron stars.

They are massively compressed neutron stars that intermittently sendout bursts of radio waves that can last for as few as two milliseconds withdark gaps lasting as long as three hours.

Supernovae remnants can leave behind pulsars or spinning neutron stars that may produce gravitational waves.

The onset of superfluidity in materials on Earth occurs at extremely low temperatures near absolute zero, but in neutron stars, it can occur at temperatures near a billion degrees Celsius.