Supernovae in Three-Dimension: A Link to Gamma-Ray Bursts

被引:0
作者
Maeda, Keiichi [1 ]
机构
[1] Max Planck Inst Astrophys, D-85741 Garching, Germany
来源
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2008年 / 8卷
关键词
supernovae: individual (SN 1998bw); gamma rays: bursts; radiative transfer; nuclear reactions; nucleosynthesis; abundances;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observational consequences of a jet-driven supernova (SN) explosion model are presented. The results are compared in detail with optical observations of SN 1998bw associated with a Gamma-Ray Burst. It is shown that the jet model is able to reproduce virtually all the optical observations available for this SN, although a spherical model fails to explain some of observed features. Because of the viewing angle effect, the required kinetic energy of the SN ejecta is reduced to similar to 2 x 10(52) erg as compared to that obtained by the previous spherical model (similar to 5 x 10(52) erg), but this is still much larger than that of a canonical SN (similar to 10(51) erg).
引用
收藏
页码:361 / 365
页数:5
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