There are two main theories concerning massive star formation, accretion and merger.
目前大质量恒星形成的理论主要有两种，即吸积说和并合说。
Massive star formation and star formation in star clusters will be very important in the future work.
未来的观测和研究重点在于：大质量恒星形成以及星团环境中的恒星形成。
Star clusters like NGC 3603 provide important clues to understanding the origin of massive star formation in the early, distant universe.
NGC3603星云给了我们一个重要的提示，让我们明白了星团在早期，遥远的宇宙里形成的原始状态。
Brightly lit with new and blue massive stars, star formation appears so rampant in NGC 1313 that it has been labeled a starburst galaxy.
伴随年轻、蓝色的大质量恒星发出的强光，NGC 1313因其中的恒星形成区蔓生而被归为星暴星系。
The recent star formation itself was likely triggered by winds and supernova explosions, from previous generations of massive stars, that swept up and compressed the molecular gas.
近期的恒星形成本身似乎由星风和超新星爆发触发，来自前代大质量恒星，清除和压缩了分子气体。
Astronomers also use massive clusters to study distant starbursts that occur when galaxies collide, igniting a flurry of star formation.
当星系碰撞，点燃了星体构造的活动时，天文学家也用团块星云来研究遥远的星体爆炸发生的情形。
The other region had ample material to form massive stars, but showed little signs of star formation, meaning that it is at one of the earliest stages yet identified in the birth of stars.
另一区域虽然拥有足以形成大质量恒星的物质，却几乎没有恒星形成的迹象，这意味着它处于目前所知的恒星形成的最早阶段之一。
Massive mergers sparked bursts of star formation when the Universe was half its age.
大规模的兼并引发了恒星形成时爆发是宇宙年龄的一半。
The massive stars in the ring are all likely less than 10 million years old, indicating the galaxy experienced a well-defined era of rapid star formation.
这些在环上的巨大恒星年龄都在10百万年以内，这指出此星系经历了快速恒星形成的明确时代。
The massive stars in the ring are all likely less than 10 million years old, indicating the galaxy experienced a well-defined era of rapid star formation.
这些在环上的巨大恒星年龄都在10百万年以内，这指出此星系经历了快速恒星形成的明确时代。
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