Should we see iron features in the AGN model of the X-ray background?

被引：3
作者：
Gilli, R
Comastri, A
Brunetti, G
Setti, G
机构：
[1] CNR, Ist Radioastron, I-40129 Bologna, Italy
[2] Osservatorio Astron Bologna, I-40126 Bologna, Italy
[3] Univ Bologna, Dipartimento Astron, I-40126 Bologna, Italy
来源：
ASTRONOMISCHE NACHRICHTEN | 1998年 / 319卷 / 1-2期
关键词：
D O I：
10.1002/asna.2123190129
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
[No abstract available]
引用
收藏
页码：65 / 65
页数：1
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