中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Numerical simulation of hot accretion flows with thermal conduction

文献类型:期刊论文

作者Wu MaoChun; Yuan Feng; Bu DeFu
刊名SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
出版日期2010
卷号53期号:1页码:168-172
关键词black hole accretion disk thermal conduction
英文摘要We report on the effects of isotropic thermal conduction in non-radiative collisionless accretion flows in two dimensions. In comparison to accretion flows without conduction, we find that the disk generally becomes cooler and thinner. Specifically, the magnitude of this effect depends on the kinetic viscosity coefficient. If it is proportional to density, the density profile of the accretion flow is flat, therefore the effect is not very obvious. But, if it is proportional to r(1/2), as is usual for the "alpha" disk description, the density profile is steeper. Therefore, the effect will be much more obvious, with the temperature profile of the accretion flow becoming much flatter. This will have important observational consequences.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Physics, Multidisciplinary
研究领域[WOS]Physics
关键词[WOS]DIMENSIONS ; GAS
收录类别SCI
语种英语
WOS记录号WOS:000280291800039
公开日期2011-06-29
源URL[http://119.78.226.72//handle/331011/13377]  
专题上海天文台_星系宇宙学重点实验室
作者单位Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
推荐引用方式
GB/T 7714
Wu MaoChun,Yuan Feng,Bu DeFu. Numerical simulation of hot accretion flows with thermal conduction[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2010,53(1):168-172.
APA Wu MaoChun,Yuan Feng,&Bu DeFu.(2010).Numerical simulation of hot accretion flows with thermal conduction.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,53(1),168-172.
MLA Wu MaoChun,et al."Numerical simulation of hot accretion flows with thermal conduction".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 53.1(2010):168-172.

入库方式: OAI收割

来源:上海天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。