NAOC Open IR
射电脉冲星锥成分的谱行为
乔国俊1; 王洪光2; 韩金林2
2000
Source Publication天体物理学报
ISSN0253-2379
Volume020Issue:004Pages:343
Abstract选取23颗双峰轮廓脉冲星,考察脉冲星射电辐射锥成分的谱行为,通过对前导和后随成分峰值强度比与频率的关系进行幂律谱拟合,给出了前后两部分的相对谱指数,结果显示,大多数脉冲星的相对谱指数集中分布在零附近,这表明,前导和后随成分的辐射本质上滑有差别;相对谱指数的近似高斯分布显示出,其辐射部位离辐射束中心距离之差具有一定的随机性。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51250
Collection中国科学院国家天文台
Affiliation1.北京大学
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
乔国俊,王洪光,韩金林. 射电脉冲星锥成分的谱行为[J]. 天体物理学报,2000,020(004):343.
APA 乔国俊,王洪光,&韩金林.(2000).射电脉冲星锥成分的谱行为.天体物理学报,020(004),343.
MLA 乔国俊,et al."射电脉冲星锥成分的谱行为".天体物理学报 020.004(2000):343.
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