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类星体的质量估计
胡佛兴
1981
Source Publication自然杂志
ISSN0253-9608
Volume4Issue:8
Abstract类星体是天体物理重大疑谜之一,质量是其重要的物理参量。本文试从“爱因斯坦天文台”发射后第一批X射线类星体资料提出对类星体质量的一种估计。首批资料共42个,其中6个给出上限X光度。分析X射线与光学波段能谱指数α_(ox)与红
Keyword质量估计 爱因斯坦天文台 天体物理 能谱指数 物理参量 类星体 红移 射线 演化效应 爱丁顿极限
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7417
Collection期刊(老文献)
Recommended Citation
GB/T 7714
胡佛兴. 类星体的质量估计[J]. 自然杂志,1981,4(8).
APA 胡佛兴.(1981).类星体的质量估计.自然杂志,4(8).
MLA 胡佛兴."类星体的质量估计".自然杂志 4.8(1981).
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