ngc的例句大全

NGC 3256 actually shows a current picture of two galaxies that are slowly colliding.

事实上,NGC3256是两个星系正缓慢地碰撞的模样.

The DNA sequence of the cloned NS 1 gene showed a 99 % homology with the DEN 2 NGC ( Genbank : AF 038403 ).

序列测定证实该基因与DEN2 ( NGC株AF038403 ) NS1基因序列有99%同源.

We report Chandra observations of the Seyfert 1.9 galaxy NGC 526 A.

报告了Seyfert1.9星系NGC526A的Chandra观测结果.

Two unraveled by the gravity of the much larger spiral, NGC 5907.

被大出许多的漩涡星系NGC5907的引力撕开之后, 这个小质量矮星系所剩下的只有两条星河了——或许还有暗物质.

Inside the nebula lies an open cluster of bright young stars designated NGC 2244.

于星云中躺著一群由明亮年轻恒星组成的疏散星团,名为NGC2244.

NGC revisits the tragedy and analyzes the ferocious storm that left six sailors dead.

然而在比赛开始后没多久,气象预报员发现有个暴风雨成形,将对赛事造成重大影响.

The picture at upper right shows a relatively calm galaxy called NGC 4145.

右上角的这张照片是相对处于平静期的4145星系.

This field spans around 60 light-years at the estimated distance of NGC 7822.

以NGC7822的估计距离推算,这幅图片的跨度约60光年.

Explanation: Big, beautiful spiral galaxy NGC 7331 is often an analog to our own Milky Way.

说明: 巨大美丽的螺旋星系NGC7331经常被认为与我们自己的银河类似.

Explanation: From our vantage point in Milky Way Galaxy, we see NGC 6946 face-on.

说明: 因为本银河系的特殊位置, 因此我们能够观测到NGC6946的正面.

These new H 2 O masers are associaned with CO molecular outflows [ 2～5 ] AFGL 5142, HH-3, AFGL 5157 , NGC 2023, RNO 73,20126 + 4104, L 1251-A.

这些新H2O脉泽是与CO分子外流源 [ 2-5 ] AFGL5142, HH - 3, AFOL5157, NGC2023,RNO73, 20126+4104, L1251 - A成协的.

Results: GC have some fatal factors from NGC.

结果: 相对于NGC,GC存在着一定的危险因素.

NGC 3372 , known as the GreatNebula in Carina , is home to massive stars and changing nebula.

NGC3372, 也就是广为人知的船底座大星云,是大量恒星和变化中的星云的大本营.

Is NGC 7582 a Starburst Galaxy?

NGC7582是一个星爆星系 吗 ?

NGC 6946 in infrared andin gas and dust, exhibiting a high star birth and death rate.

NGC6946充满气体以及尘埃, 有很强的红外线波段的发光,因此有很高的星球出生率以及死亡率.

NGC 1512 is a barred spiral galaxy in the southern constellation of Horologium.

NGC1512是一个处在南天时钟座的棒旋星系.

Images of NGC 3132 reveal two stars close together within the nebulosity, one of 10th magnitude, the other 16th.

在NGC3132朦胧的影像中显示有两颗紧密靠在一起的恒星，一颗的视星等是10等，另一颗是16等。

There was no significant difference observed for all measured indexes ( P> 0.05) between LGC and NGC groups at baseline.

基线时，LGC组与NGC组间各观察指标均无明显统计学差异（P＞0.05）。

Grand spiral galaxy NGC 1232, captured in detail by one of the new Very Large Telescopes, is a good example.

壮丽的螺旋星系NGC1232就是一个很好的例子。上面这张NGC1232影像，是由一部极大望远镜所拍摄的，影像中可以清楚地看见这个星系壮丽的漩涡臂。