| 赛佛特星系金属丰度的求解 |
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| 引用本文： | 史菲,刘玉燕.赛佛特星系金属丰度的求解[J].华北航天工业学院学报,2014(1):1-2,6. |
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| 作者姓名： | 史菲 刘玉燕 |
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| 作者单位： | [1]北华航天工业学院基础科学部,河北廊坊065000 [2]北华航天工业学院计算机科学与工程系,河北廊坊065000 |
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| 基金项目： | 北华航天工业学院博士专项基金（BKY-2013-07） |
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| 摘 要： | 对于赛佛特星系(文中简称WR星系),作为一种重要的活动星系的类型,求其金属丰度对我们具有重要的意义,本文将详细介绍计算HII区星系金属丰度的方法,并据此计算若干赛佛特星系的金属丰度。
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| 关 键 词： | HII 星系 金属丰度 |
Metallicity Determination Methods for WR Galaxies |
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| SHI Fei,LIU Yu-Yan.Metallicity Determination Methods for WR Galaxies[J].Journal of North China Institute of Astronautic Engineering,2014(1):1-2,6. |
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| Authors: | SHI Fei LIU Yu-Yan |
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| Institution: | 1. Fundanmental Science Department, North China Institute of Aerospace Engineering, Langfang 065000, China; 2. Computer Science ＆ Engineering Department, North China Institute of Aerospace Engineering, Langfang 065000, China) |
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| Abstract: | The paper presents the methods of metallicity determination of galaxy, mainly for oxygen abundance. Among them, the methods based on radiation mechanism are analyzed in detail because of a firm theoretical basis. The other methods, such as dynamic metallicity, stellar photometry, image, X-Ray, stellar population synthesis, are also given as a brief introduction. |
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| Keywords: | HII galaxy metallicity |
| 本文献已被 CNKI 维普 等数据库收录！ |
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