Chinese | English
IMECH-IR  > 力学所知识产出(1956-2008)
星系密度波的共转奇异性
胡文瑞
Source Publication科学通报
1979
Volume24Issue:11Pages:351-360
ISSN0023-074X
Abstract<正> 在线性密度波理论中,主要有三个奇异半径,即共转奇异性和内、外Lindblad共振。这些奇异区域对星系线性密度波有重要影响。共转圈一般位于星系盘的适中位置,对它的奇异性影响应进行分析。我们曾经指出,若用矩方程来描述恒星的集体行为,假设弥散速度为一标
Keyword密度波 奇异性 共转 星系盘 矩方程 集体行为 重要影响 区域对 线性
Language中文
Document Type期刊论文
Identifierhttp://dspace.imech.ac.cn/handle/311007/38688
Collection力学所知识产出(1956-2008)
Corresponding Author胡文瑞
Recommended Citation
GB/T 7714		 胡文瑞. 星系密度波的共转奇异性[J]. 科学通报,1979,24,11,:351-360.
APA 胡文瑞.(1979).星系密度波的共转奇异性.科学通报,24(11),351-360.
MLA 胡文瑞."星系密度波的共转奇异性".科学通报 24.11(1979):351-360.
Files in This Item: Download All
File Name/Size DocType Version Access License
ja006.pdf（179KB） 开放获取--View Download
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Lanfanshu
Similar articles in Lanfanshu
[胡文瑞]'s Articles
Baidu academic
Similar articles in Baidu academic
[胡文瑞]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[胡文瑞]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: ja006.pdf
Format: Adobe PDF
This file does not support browsing at this time
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.