4.8 Article

Detection of Pristine Gas Two Billion Years After the Big Bang

期刊

SCIENCE
卷 334, 期 6060, 页码 1245-1249

出版社

AMER ASSOC ADVANCEMENT SCIENCE
DOI: 10.1126/science.1213581

关键词

-

资金

  1. Humboldt Foundation
  2. NSF [AST0548180]
  3. W. M. Keck Foundation

向作者/读者索取更多资源

In the current cosmological model, only the three lightest elements were created in the first few minutes after the Big Bang; all other elements were produced later in stars. To date, however, heavy elements have been observed in all astrophysical environments. We report the detection of two gas clouds with no discernible elements heavier than hydrogen. These systems exhibit the lowest heavy-element abundance in the early universe, and thus are potential fuel for the most metal-poor halo stars. The detection of deuterium in one system at the level predicted by primordial nucleosynthesis provides a direct confirmation of the standard cosmological model. The composition of these clouds further implies that the transport of heavy elements from galaxies to their surroundings is highly inhomogeneous.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.8
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据