星际碳预算以及碳在尘埃和大分子中的作用
1Center for Astrophysics and Space Astronomy, University of Colorado, Boulder 80309, USA.
概括
太阳的碳含量明显高于其他恒星,影响了我们对银河系组成和超新星核合成的理解. 这一发现挑战了现有的模型,并表明星际尘埃形成可用的碳较少.
科学领域:
- 天文学和天体物理学
- 恒星的组成 恒星的组成
- 太空化学 太空化学
背景情况:
- 发表的恒星组成数据表明,与其他银河系恒星相比,太阳的碳含量更高.
- 代表性的银河系恒星显示大约225个碳原子每10^6个原子,而太阳显示的值从350到470.
研究的目的:
- 分析太阳过多的碳对天体物理模型的影响.
- 为了重新评估标准.
主要方法:
- 分析已发表的恒星组成数据.
- 太阳碳丰度与银河系和星际平均值的比较.
- 对核合成和尘埃形成模型的影响评估.
主要成果:
- 太阳的碳丰度比银河系平均水平 (每106H的225个) 高得多 (350-470个每106H).
- 太阳系中其他元素的增加量表明它们与超新星事件有关.
- 银河系的碳预算受到限制,这可能会使一些星际尘埃模型变得不可思议.
结论:
- 太阳的高碳含量需要对超新星核合成模型进行修订.
- 由于太阳系的丰富性",宇宙"组成标准需要修改.
- 减少银河系碳的可用性给当前的星际尘埃形成理论带来了挑战.
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