The fate of the first galaxies. II. Effects of radiative feedback

被引:182
作者
Ricotti, M
Gnedin, NY
Shull, JM
机构
[1] Univ Colorado, Ctr Astrophys & Space Astron, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA
[2] Univ Colorado, JILA, Boulder, CO 80309 USA
[3] Univ Colorado, Natl Inst Stand & Technol, Boulder, CO 80309 USA
关键词
cosmology : theory; galaxies : dwarf; galaxies : evolution; galaxies : formation; galaxies : high-redshift; intergalactic medium;
D O I
10.1086/341256
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use three-dimensional cosmological simulations with radiative transfer to study the formation and evolution of the first galaxies in a LambdaCDM cosmology. The simulations include continuum radiative transfer using the optically thin variable Eddington tensor ( OTVET) approximation and line radiative transfer in the H-2 Lyman-Werner bands of the UV background radiation. Chemical and thermal processes are treated in detail, particularly the ones relevant for H-2 formation and destruction. We find that the first luminous objects ("small-halo objects") are characterized by bursting star formation ( SF) that is self-regulated by a feedback process acting on cosmological instead of galactic scales. The global SF history is regulated by the mean number of ionizing photons that escape from each source, epsilon(UV) (f(esc)). It is almost independent of the assumed SF efficiency parameter, epsilon(*), and the intensity of the dissociating background. The main feedback process that regulates the SF is the reformation of H-2 in front of H II regions and inside relic H II regions. The H II regions remain confined inside laments, maximizing the production of H-2 in overdense regions through cyclic destruction/reformation of H-2. If epsilon(UV) (f(esc)) > 10(-7)/epsilon(*), the SF is self-regulated, photoevaporation of small-halo objects dominates the metal pollution of the low-density intergalactic medium, and the mass of produced metals depends only on (f(esc)). If epsilon(UV) (f(esc)) less than or similar to 10(-7)/epsilon(*), positive feedback dominates, and small-halo objects constitute the bulk of the mass in stars and metals until at least redshift z similar to 10. Small-halo objects cannot reionize the universe because the feedback mechanism confines the H II regions inside the large-scale structure laments. In contrast to massive objects ( large halos), which can reionize voids, small-halo objects partially ionize only the dense laments while leaving the voids mostly neutral.
引用
收藏
页码:49 / 67
页数:19
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