NAOC Open IR
Mrk 421中TeV和X射线爆发的相关性
Britzen S1; Krichbaum T1; Witzel A1; 钱善2; 张喜镇2; Kraus A1
1998
Source Publication天体物理学报
ISSN0253-2379
Volume018Issue:001Pages:17
Abstract用同步-自康普顿机制(SSC)来解释1994年5月在BLlac天体Mrk421中观测到的TeV-X射线爆发,认为此Tex-X射线爆发是由一个高能成分产生的,它具有平坦的电子能量分布,其低能段上能谱指数αe≈0.25,这个爆发成分独立另一个低能成分(或宁静成分)此宁静成分具有较陡的电子能量分布,它产生宁静态的辐射能谱。大多数射电爆发表明电子能量分布有坦谱,能谱指数αe≈0.2-0.4,与这个事实一起
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/50525
Collection中国科学院国家天文台
Affiliation1.德国马普学会射电天文学研究所
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
Britzen S,Krichbaum T,Witzel A,等. Mrk 421中TeV和X射线爆发的相关性[J]. 天体物理学报,1998,018(001):17.
APA Britzen S,Krichbaum T,Witzel A,钱善,张喜镇,&Kraus A.(1998).Mrk 421中TeV和X射线爆发的相关性.天体物理学报,018(001),17.
MLA Britzen S,et al."Mrk 421中TeV和X射线爆发的相关性".天体物理学报 018.001(1998):17.
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
[Britzen S]'s Articles
[Krichbaum T]'s Articles
[Witzel A]'s Articles
Baidu academic
Similar articles in Baidu academic
[Britzen S]'s Articles
[Krichbaum T]'s Articles
[Witzel A]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Britzen S]'s Articles
[Krichbaum T]'s Articles
[Witzel A]'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.