中文

对第一代恒星和类星体的经验约束

天体物理学 2009-10-31 v2

摘要

对宇宙中第一代恒星和类星体的经验研究很快将变得可行。下一代太空望远镜将提供对红移z>10的亚星系对象进行的直接成像和光度测量,而微波各向异性实验,如MAP或Planck,将对由于这些源导致的星际介质电离历史施加约束。我们描述了这些未来仪器将可检测的预期信号。

关键词

引用

@article{arxiv.astro-ph/9811395,
  title  = {Empirical Constraints on the First Stars and Quasars},
  author = {Zoltan Haiman and Avi Loeb},
  journal= {arXiv preprint arXiv:astro-ph/9811395},
  year   = {2009}
}

备注

14 pages, invited contribution to Proc. of 9th Annual October Astrophysics Conference in Maryland, "After the Dark Ages: When Galaxies Were Young (the Universe at 2 < z < 5", College Park, October 1998