Fossil records of cosmic reionization in galactic stellar halos

Kenji Bekki, Masashi Chiba

研究成果: Review article査読

13 被引用数 (Scopus)

抄録

Galactic stellar halos have long been considered to contain fossil information on the early dynamical and chemical evolution of galaxies. We propose that the surface brightness distributions of old stellar halos contain the influence of reionization on early formation histories of galaxies. By assuming that reionization significantly suppresses star formation in small subgalactic clumps virialized after reionization redshift (zreion), we first numerically investigate how the structural and kinematical properties of stellar halos that formed from the merging of these subgalactic clumps depend on zreion. We then discuss what observable properties of galactic stellar halos offer us; we also discuss the fossil records of reionization influence on hierarchical formation of halos based on the current results of numerical simulations. We specifically suggest that both the half-light radius of stellar halos and the slope of their surface brightness profile contain useful information regarding the times in which star formation in subgalactic clumps were significantly influenced by reionization. By using the simulated surface brightness distributions of galactic stellar halos for models with different zreion, we also discuss how wide-field imaging studies of extragalactic halos will help us to elucidate the epoch of cosmic reionization.

本文言語English
ページ(範囲)L107-L110
ジャーナルAstrophysical Journal
625
2 II
DOI
出版ステータスPublished - 2005 6 1

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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