PMO OpenIR  > 期刊(老文献)
类星体的光度演化
龚树模 ; 夏昌立
1982
Source Publication天文学报
ISSN0001-5245
Volume23Issue:3Pages:243-254
Abstract本文采用作者提出的大气密度分析模型,导出了人造地球卫星大气阻力摄动新的计算公式,它适用于0≤e≤0.3的各种近地卫星。
Keyword类星体 光度演化 绝对星等 标准烛光 视星等 光度距离 哈勃图 哈勃关系 减速因子 红移
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7471
Collection期刊(老文献)
Recommended Citation
GB/T 7714
龚树模,夏昌立. 类星体的光度演化[J]. 天文学报,1982,23(3):243-254.
APA 龚树模,&夏昌立.(1982).类星体的光度演化.天文学报,23(3),243-254.
MLA 龚树模,et al."类星体的光度演化".天文学报 23.3(1982):243-254.
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