NAOC Open IR
吸积盘整体结构的统一描述
赵永恒1; 陈兴明2; 吴学兵1
1996
Source Publication天体物理学报
ISSN0253-2379
Volume016Issue:003Pages:221
Abstract在考虑径向对流和不同光学厚度的基础上,我们采用一般的辐射冷假设,在统一的框架内考察了吸积盘的整体结构,对α模型,我们发现在不同盘区在不同的整体结构,在吸积率较低时,存在三种类型解,光学厚的局部辐射冷解,光学薄的局部致冷解,光学薄的对流致冷解,这些解在盘内较大范围内都存在且互不交叉,但在吸积率较高和粘滞系数较大时,两种局部致冷解会相互交叉,而对流为主的解在所有盘区都稳定存在,另一方面,在吸积率较高和
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/53053
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.Geteberg University and Chaimers University of Technology
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
赵永恒,陈兴明,吴学兵. 吸积盘整体结构的统一描述[J]. 天体物理学报,1996,016(003):221.
APA 赵永恒,陈兴明,&吴学兵.(1996).吸积盘整体结构的统一描述.天体物理学报,016(003),221.
MLA 赵永恒,et al."吸积盘整体结构的统一描述".天体物理学报 016.003(1996):221.
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