galactic disk 中文意思是什麼
galactic disk
解釋
銀盤-
Van den bosch is particularly intrigued by the formation of disk galaxies and of massive black holes in galactic centers
范登柏希特別著迷於盤形星系與星系中心超大質量黑洞的形成過程。 -
Which is spherical and even larger than the galactic disk. the halo consists of old stars, some in the globular clusters, and interstellar matter
銀冕內主要為年老的星,它們有些在球狀星團內,有些則在星際物質中游蕩。 -
The galaxy ' s central region is called the galactic bulge because the stars form a ball a few thousand light years in diameter that extends above and below the disk of the galaxy
星系的中心區域叫做核球,原因是恆星組成了直徑幾千光年的球體,膨脹到星系盤上下兩側。 -
This letter aiming at this respect, hints for neutron capture element are derived : 1. based on the adopted galactic evolution scenario, together with the three - zone multi - phase model, observational features of the solar vicinty region can be well reproduced. among those are particuly g - dwarf problem. the g - dwarf problem in halo and thin - disk can be solved
本文正是從這方面著手,對中子俘獲元素進行了研究,得到如( 1 ) r過程元素核合成產量隨著超新星前身星的質量的增加而單調增加, r -過程核合成場所是sn ,質量范圍是18m _ m 50m _ ,這與mathews 、 tsujimoto和travaglio等人的結果完全不同。 -
As we continue outward into the farthest reaches of the galactic disk, the stars are separated by dozens, then hundreds, of light - years, and the interstellar gas thins out 100 - fold
當我們繼續朝銀盤最外沿前進,恆星間的距離從幾十光年延長為幾百光年,而星際氣體則變稀薄100倍。
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