RCW120 fragmentation at 0.01pc scale
收藏B2FIND2026-04-04 收录
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Little is known about how high-mass stars form. Around 30% of the young high-mass stars in the Galaxy are observed at the edges of ionized (HII) regions. Therefore these are...
目前学界对大质量恒星(high-mass stars)的形成机制仍知之甚少。在银河系(Galaxy)中,约30%的年轻大质量恒星被观测到处于电离氢区(ionized (HII) regions)的边缘。因此此类恒星为……



