NAOC Open IR
候选射电脉冲星的预测
吴鑫基1; 田文武2; 张喜镇2
1999
Source Publication天体物理学报
ISSN0253-2379
Volume019Issue:004Pages:375
Abstract对已知脉冲星大样本的统计和分析表明,绝大多数脉冲星的线偏振大于10%,谱指数低于-1,比较了脉冲星和射电类星体及致密陡谱源的频谱和偏振特性的差别,以高线偏振,高谐系数,高银纬及在低频下较低流量等作为射电脉冲星候选者的判据,从新近释放的VLA巡天和WSRT巡天结果中挑选出一个较粗的候选脉冲星样本。进一步考虑近期在部分天区中已作过高灵敏度的脉冲星巡天,所有落入这些天区内的候选源也都从本样本中排出,以候
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51584
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
吴鑫基,田文武,张喜镇. 候选射电脉冲星的预测[J]. 天体物理学报,1999,019(004):375.
APA 吴鑫基,田文武,&张喜镇.(1999).候选射电脉冲星的预测.天体物理学报,019(004),375.
MLA 吴鑫基,et al."候选射电脉冲星的预测".天体物理学报 019.004(1999):375.
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