NAOC Open IR
ngc7582是一个星爆星系吗
苏步美; 高亦菲; 李永生
1999
Source Publication天体物理学报
ISSN0253-2379
Volume019Issue:004Pages:353
Abstract棒旋星系NGC7582的光学发射线显示出它具有Seyfert2和星爆星系的双重特点。本文利用射电和红外观测数据对它中心区附近的性质进行了研究。结果表明NGC7582中心附近可能存在着一个活动性很强的恒星形成区,恒星的形成率比银河系高得多,星爆对这个Seyfert2星系的性质起了重要作用。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/44138
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
苏步美,高亦菲,李永生. ngc7582是一个星爆星系吗[J]. 天体物理学报,1999,019(004):353.
APA 苏步美,高亦菲,&李永生.(1999).ngc7582是一个星爆星系吗.天体物理学报,019(004),353.
MLA 苏步美,et al."ngc7582是一个星爆星系吗".天体物理学报 019.004(1999):353.
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