中子星的吸积流动

IMECH-IR > 力学所知识产出(1956-2008)

	中子星的吸积流动
	胡文瑞
Source Publication	天体物理学报
	1984
Volume	4 Issue:3 Pages:173-183
ISSN	0253-2379
Abstract	本文分析中子星的吸积流动,其中磁轴与自转轴重合.吸积盘内缘区域的波阻将使盘内的角速度偏离开普勒速度而减小,引力势能使流体加热和加速.吸积盘中有两类流动.完全亚声速流动的引力势能主要使吸积流加热.另一种流动有跨声速过渡和激波.这两种流动都表明,吸积盘的高温区域都位于过渡区中,而外部区域中气体温度不高.还计算了中子星磁层中的吸积流动.在极区距几个中子星半径处,气体被急剧加热,产生X射线辐射,形成热斑.这些结果与中子星吸积流动的主要特征一致.
Keyword	吸积盘吸积流中子星过渡区磁层亚声速流声速点远区波阻
Language	中文
Document Type	期刊论文
Identifier	http://dspace.imech.ac.cn/handle/311007/37566
Collection	力学所知识产出(1956-2008)
Corresponding Author	胡文瑞
Recommended Citation GB/T 7714	胡文瑞. 中子星的吸积流动[J]. 天体物理学报,1984,4,3,:173-183.
APA	胡文瑞.(1984).中子星的吸积流动.天体物理学报,4(3),173-183.
MLA	胡文瑞."中子星的吸积流动".天体物理学报 4.3(1984):173-183.

Related Services

Bookmark

Lanfanshu

Similar articles in Bing Scholar

Terms of Use

No data!

Social Bookmark/Share

File name:	Paper0994.caj
Format:	Unknown

This file does not support browsing at this time

All comments (0)

No comment.

The comment function is only available to registered usersLog In

If you have any objections to this item, please fill out the form below and the administrator will contact you as soon as possible.
Content:
Email：	*
Institution:
Verification Code:	Refresh

Any comments and suggestions are welcomed.
Title:	*
Content:
Email：	*
Verification Code:	Refresh

中国科学院力学研究所机构知识库