NAOC Open IR
Blazar天体射电爆发的持续注入喷流模型
钱善
1996
Source Publication天体物理学报
ISSN0253-2379
Volume016Issue:001Pages:15
Abstract为了解释Blazar天体射电爆发的普遍演化特性,本文提出一个持续注入的喷流模型。假定在喷流基底上以相对论性速度持续地注入相对论等离子体(由磁场和相对论电子组成)。这一等离子体在沿喷流向外运动时经受绝热膨胀损耗。理论计算表明,射电爆发的频谱演化具有Valtaoja等人所建议的典型的3阶段演化形式。它们非常好地重现了Blazar天体中观测到的射电爆发的普遍行为。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/46042
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
钱善. Blazar天体射电爆发的持续注入喷流模型[J]. 天体物理学报,1996,016(001):15.
APA 钱善.(1996).Blazar天体射电爆发的持续注入喷流模型.天体物理学报,016(001),15.
MLA 钱善."Blazar天体射电爆发的持续注入喷流模型".天体物理学报 016.001(1996):15.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[钱善]'s Articles
Baidu academic
Similar articles in Baidu academic
[钱善]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[钱善]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

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