NAOC Open IR
尘埃辐射转移模型
陈培生; 何金华
2000
Source Publication天文学进展
ISSN1000-8349
Volume018Issue:003Pages:249
Abstract尘埃辐射转移模型对解释和探索宇宙中众多的多尘埃天体的观测现象可发挥重要的作用。目前所见的四种球对称系统中的尘埃辐射转移方法可被总结为:二流Eddington近似模型方法,Eddington因子迭代模型方法、射线跟踪法和Monte-Carlo模型方法,除了第一种方法外,其余方法在原理上都没有近似性。现在使用最多的是后两种方法。Monte-Carlo方法是其中最灵活的一种,它可被用于对非球对称系统的辐
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/53080
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
陈培生,何金华. 尘埃辐射转移模型[J]. 天文学进展,2000,018(003):249.
APA 陈培生,&何金华.(2000).尘埃辐射转移模型.天文学进展,018(003),249.
MLA 陈培生,et al."尘埃辐射转移模型".天文学进展 018.003(2000):249.
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