NAOC Open IR
类星体色指数随红移的变化
陈建生; 樊晓晖
1994
Source Publication天体物理学报
ISSN0253-2379
Volume014Issue:003Pages:197
Abstract本文讨论了类星体各光谱特征对其色指数的影响以及色指数随红移的变化,随着红移的增加,位于Lya发射线短波方向的各种吸收特征进入了可见光区,内禀的禀的幂律谱和发射线强度的分布对类星体色指数及其弥散的影响将是次要的,各种吸收系统的作用将改变类星体色指数随红移变化的趋势,其中,Lyman系限吸收系统的影响最大,利用IUE观测的类星体光谱求得色指数随红移的变化,对上述结果进行了验证。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/42145
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
陈建生,樊晓晖. 类星体色指数随红移的变化[J]. 天体物理学报,1994,014(003):197.
APA 陈建生,&樊晓晖.(1994).类星体色指数随红移的变化.天体物理学报,014(003),197.
MLA 陈建生,et al."类星体色指数随红移的变化".天体物理学报 014.003(1994):197.
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