bulges-galaxies

基本解釋

The assemblage of all galaxies; the entire physical universe.
總星系所有星系的總稱; 整個(gè)自然宇宙
Bulges and elliptical galaxies (that is, diskless bulges) form when galaxies collide and merge.
當(dāng)星系碰撞合并時(shí)形成了橢圓星系。
In sharp contrast to bulges, the properties of disk galaxies do not correlate with BH masses.
與橢圓星系形成鮮明對(duì)比，漩渦星系的特質(zhì)與黑洞質(zhì)量沒有直接聯(lián)系。
Yet, high resolution images, using Hubble Space Telescope reveal that many bulges have properties that are more like spiral galaxies.
然而，在高解析度的影像下，使用哈柏太空望遠(yuǎn)鏡揭露出許多球核也具有與螺旋星系相同的特性。
"The black holes in these young galaxies are much more massive compared to the bulges than those seen in the nearby universe.
“相對(duì)于凸起物來說，在這些早期的星系中的黑洞比在附近銀河系看到的要大得很多”。