PMO OpenIR  > 期刊(老文献)
脉冲星的制动系数
杭恒荣 ; 王德焴
1984
Source Publication天文学报
ISSN0001-5245
Volume25Issue:2Pages:107-111
Abstract本文根据迄今为止所有发表的白光耀斑观测结果和它们对应的H_α耀斑、射电爆发、X射线爆、质子事件以及电离层等有关资料,对白光耀斑的特性进行了讨论,并检查了我台多年来观测的耀斑光谱底片,发现大约有5%的耀斑光谱资料中呈现出有变化的白光连续辐射,它们中有些只对应于很小级别的H_α耀斑。本文由此对白光辐射的起源问题提出一些设想。
Keyword蟹状星云脉冲星 制动系数 统计分析 磁偶极辐射 磁偶极矩 统计结果 能量损失 斜率 能损 角速度
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7541
Collection期刊(老文献)
Recommended Citation
GB/T 7714
杭恒荣,王德焴. 脉冲星的制动系数[J]. 天文学报,1984,25(2):107-111.
APA 杭恒荣,&王德焴.(1984).脉冲星的制动系数.天文学报,25(2),107-111.
MLA 杭恒荣,et al."脉冲星的制动系数".天文学报 25.2(1984):107-111.
Files in This Item:
File Name/Size DocType Version Access License
1984566脉冲星的制动系数.pdf(1429KB) 开放获取LicenseView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[杭恒荣]'s Articles
[王德焴]'s Articles
Baidu academic
Similar articles in Baidu academic
[杭恒荣]'s Articles
[王德焴]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[杭恒荣]'s Articles
[王德焴]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 1984566脉冲星的制动系数.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

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