早期恒星形成的低质量遗迹
R Schneider1, A Ferrara, R Salvaterra
1Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy.
Nature
|April 25, 2003
概括
最早的恒星没有金属形成,有利于大质量恒星. 然而,极低金属度气体中的尘埃使今天的低质量恒星的形成成为可能.
科学领域:
- 天文学 天文学
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
背景情况:
- 大爆炸后形成的第一批恒星显著影响了随后的恒星世代.
- 以前的研究表明,大质量恒星 (高达100太阳质量) 在没有金属的条件下形成,而低质量恒星需要一些金属丰富.
研究的目的:
- 研究尘埃在早期宇宙中低质量恒星形成中的作用.
- 了解可观测的低质量恒星形成所需的最小金属度.
主要方法:
- 对已知最缺乏铁的恒星进行分析.
- 研究极低金属度气体中尘埃的存在和影响.
主要成果:
- 最缺乏铁的恒星表明,即使在非常低的金属度下,尘埃也存在.
- 这种尘埃对于冷却气体至关重要,使分子云的碎片化成为可能.
- 碎片化导致质量较低的第二代恒星的形成.
结论:
- 尘埃,不仅仅是金属,在早期恒星形成中起着关键作用.
- 尘埃的存在促进了低质量恒星的形成,这些恒星可以存活到今天.
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