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球状星团中黑洞附近星的投影密度分布
谢光中; 鲍梦贤; 邓立吾; 张家铝
Source Publication天文学报
1981-03
Volume22Issue:1Pages:100-106
Contribution Rank第1完成单位
Indexed By其他
Abstract本文用广义相对论讨论了球状星团中黑洞附近星的密度分布。结果表明:1.星的密度分布n不仅是径向坐标,的函数,而且是比热比r的函数。2.Peeblet和J.N.Bacall等人关于n的结果是本文的一种特殊情况(r≤4/3)。此外,我们还用数字积分得出了星的投影密度分布曲线,可供观测对比验证。
Language中文
Subject Area天文学
Subtype期刊论文
ISSN0001-5245
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/7061
Collection星系研究组
Recommended Citation
GB/T 7714
谢光中,鲍梦贤,邓立吾,等. 球状星团中黑洞附近星的投影密度分布[J]. 天文学报,1981,22(1):100-106.
APA 谢光中,鲍梦贤,邓立吾,&张家铝.(1981).球状星团中黑洞附近星的投影密度分布.天文学报,22(1),100-106.
MLA 谢光中,et al."球状星团中黑洞附近星的投影密度分布".天文学报 22.1(1981):100-106.
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