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Fe离子M壳层不可分辨跃迁系不透明度研究

董富通 王菲鹿 仲佳勇 赵刚

物理学报2012,Vol.61Issue(16):153-158,6.
物理学报2012,Vol.61Issue(16):153-158,6.

Fe离子M壳层不可分辨跃迁系不透明度研究

Research on the opacity of Fe M-shell unresolved transition array

董富通 1王菲鹿 1仲佳勇 1赵刚1

作者信息

  • 1. 中国科学院国家天文台,北京100012
  • 折叠

摘要

Abstract

M-shell unresolved transition array of iron is an important diagnostic tool of the X-ray spectrum of active galactic nuclei. This array is measured in the laboratory, and compared with several theoretical models. In the present paper, we introduce a detailed line counting model. With this model, we simulate the experimental spectra, and the comparison shows a good agreement. We also calculate the absorption spectra in a temperature range of 10-50 eV.

关键词

活动星系核/铁M壳层不可分辨跃迁系/细致谱线模型

Key words

active galactic nuclei/Fe M-shell unresolved transition array/detailed line counting model

分类

数理科学

引用本文复制引用

董富通,王菲鹿,仲佳勇,赵刚..Fe离子M壳层不可分辨跃迁系不透明度研究[J].物理学报,2012,61(16):153-158,6.

基金项目

国家自然科学基金(批准号:11173032,11103040,11135012)资助的课题. ()

物理学报

OA北大核心CSCDCSTPCDSCI

1000-3290

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