merging star

基本解釋

Arch also allows merging of changes from upstream repositories with star-merge.
Arch 還允許用 star-merge 合并來(lái)自上游存儲(chǔ)庫(kù)的變更。
In 2006 Hubble captured the Antennae galaxies merging, and billions of star births beginning in the midst of the collision.
2006年哈勃望遠(yuǎn)鏡捕捉到了雙天線星系的合并過(guò)程，在此次碰撞中誕生了數(shù)十億顆新星。
One of the brightest sources in the infrared sky, the merging galaxies spew distorted tidal tails of stars, gas, and dust and undergo frantic bursts of star formation.
這個(gè)星系對(duì)是紅外光波段天空最亮的光源之一，它們噴出由恒星、云氣和塵埃所組成的扭曲潮汐尾，而本內(nèi)部也出現(xiàn)劇烈的恒星誕生活動(dòng)。
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