Modeling the emission line and ionizing properties of primeval galaxies

被引:0
|
作者
Schaerer, Daniel [1 ]
Verhamme, Anne [1 ]
机构
[1] Univ Geneva, Observ Geneva, CH-1290 Sauverny, Switzerland
来源
FIRST STARS III | 2008年 / 990卷
关键词
pop III stars; galaxies; re-ionization; lyman-alpha;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a short overview of predictions from two modeling tools, an evolutionary synthesis code for metallicities from Z = 0 (Pop III) to solar and a general purpose 3D Ly alpha + continuum radiation transfer code. These allow us to predict the ionizing and emission line properties of objects such as star bursts and primeval galaxies, and to predict consistently Lya line strengths and profiles taking radiation transfer, ISM geometry, dust etc. into account.
引用
收藏
页码:204 / 206
页数:3
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