SN 1987A: 3D simulations of collision with the ring

被引：0
|
作者：
Maeda, K [1 ]
Nomoto, K [1 ]
Nakasato, N [1 ]
Suzuki, T [1 ]
机构：
[1] Univ Tokyo, Dept Astron, Sch Sci, Tokyo, Japan
来源：
NEUTRON STARS IN SUPERNOVA REMNANTS | 2002年 / 271卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We simulate the collision between the ejecta of SN 1987A and circumstellar material, and calculate the X-ray emission. To reproduce observations, the explosion energy and the number density of the H II region are constrained to be similar to 1.4 x 10(51) erg and similar to 100 amu cm(-3), respectively. The density of the hot spot should be similar to that of the ring (similar to 10(4) amu cm(-3)) to be consistent with the observed X-ray luminosity. In the near future, the blast wave will reach the dense ring, and the ring will be brightened in X-rays becoming more luminous than 10(36) ergs s(-1).
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页码：379 / 382
页数：4
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