Cosmic Reionization On Computers: Reionization Histories of Present-day Galaxies

被引:7
|
作者
Zhu, Hanjue [1 ]
Avestruz, Camille [2 ,3 ]
Gnedin, Nickolay Y. [2 ,4 ,5 ]
机构
[1] Univ Chicago, Chicago, IL 60637 USA
[2] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[3] Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 USA
[4] Fermilab Natl Accelerator Lab, Particle Astrophys Ctr, POB 500, Batavia, IL 60510 USA
[5] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
来源
ASTROPHYSICAL JOURNAL | 2019年 / 882卷 / 02期
基金
美国国家科学基金会;
关键词
dark ages; reionization; first stars; galaxies: high-redshift; methods: numerical; INHOMOGENEOUS REIONIZATION; COSMOLOGY;
D O I
10.3847/1538-4357/ab3794
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine the reionization history of present-day galaxies by explicitly tracing the building blocks of halos from the Cosmic Reionization On Computers project. We track dark matter particles that belong to z = 0 halos and extract the neutral fractions at corresponding positions during rapid global reionization. The resulting particle reionization histories allow us to explore different definitions of a halo's reionization redshift and to account for the neutral content of the interstellar medium. Consistent with previous work, we find a systematic trend of reionization redshift with mass-present day halos with higher masses have earlier reionization times. Finally, we quantify the spread of reionization times within each halo, which also has a mass dependence.
引用
收藏
页数:5
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