NAOC Open IR
爱因斯坦探针卫星的核塌缩超新星激波暴探测
邓劲松1; 王祥玉2
2018
Source Publication中国科学物理学力学天文学
ISSN1674-7275
Volume048Issue:003Pages:039506
Abstract在核塌缩超新星爆发过程中,当辐射主导的爆炸激波传播到前身星表面附近时,高温辐射逃逸形成激波暴,是超新星最早的电磁信号.激波暴热辐射以紫外和软X射线光子为主,持续时间短暂(~10–1000 s),仅有几个疑似观测事例.爱因斯坦探针卫星开展的大视场、高灵敏度的软X射线快速全天巡天,预期每年将获得几十颗II-P型超新星的激波暴光变曲线,对蓝超巨星爆发和Ib/Ic型超新星的激波暴合计也可能有一到数颗的年探测率,有望用于限制前身星类型、爆前物质损失、超新星爆发机制等.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47059
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.南京大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
邓劲松,王祥玉. 爱因斯坦探针卫星的核塌缩超新星激波暴探测[J]. 中国科学物理学力学天文学,2018,048(003):039506.
APA 邓劲松,&王祥玉.(2018).爱因斯坦探针卫星的核塌缩超新星激波暴探测.中国科学物理学力学天文学,048(003),039506.
MLA 邓劲松,et al."爱因斯坦探针卫星的核塌缩超新星激波暴探测".中国科学物理学力学天文学 048.003(2018):039506.
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