NAOC Open IR
Blazar天体中光学射电大爆发的频谱演化
钱善
1997
Source Publication天文学报
ISSN0001-5245
Volume038Issue:003Pages:239
Abstract本文讨论Blazar天体中光学射电大爆发频谱演化的理论模型,考虑沿喷流传播的相对论性激波所注入或加速的相对论性电子,受到康普顿、同步辐射和绝热膨胀三种损耗,并计及相对论电子能谱的高能截断。假定喷油轴线与观测者方向构成很小角度。文中给出了大爆发频谱三阶段连续演化的特性,即康普顿阶段,同步辐射阶段和绝热膨胀阶段的爆发特性。频谱演化用(Sm-νm)关系表达,它与一些Blazar天体中观测到的典型形式相符
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/38509
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
钱善. Blazar天体中光学射电大爆发的频谱演化[J]. 天文学报,1997,038(003):239.
APA 钱善.(1997).Blazar天体中光学射电大爆发的频谱演化.天文学报,038(003),239.
MLA 钱善."Blazar天体中光学射电大爆发的频谱演化".天文学报 038.003(1997):239.
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