Radio to TeV gamma‐ray emission from SN 1006 and shock acceleration around its rim
Radio to TeV gamma‐ray emission from SN 1006 and shock acceleration around its rim
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SN 1006 发射的无线电至 TeV 伽马射线及其边缘周围的冲击加速度
DOI：
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发表时间：
1999
期刊：
影响因子：
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通讯作者：
T. Tanimori
中科院分区：
文献类型：
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作者：
T. Naito;T. Yoshida;M. Mori;T. Tanimori
利用逆康普顿辐射（IC）和π°衰变过程研究了SN 1006的多波长光谱。我们的结果匹配以及一个基于IC工艺，在以前的论文中讨论。这些拟合使我们能够准确地确定冲击周围的物理参数。得到的磁场强度为4 ± 1 μG，粒子的最大加速能量为E_（max）= 51（B/4μG）-0.5TeV。所需电子的能量密度超过磁场的能量密度，因此系统可能不处于均分状态。
We examine the multi-wave-length spectrum of SN1006 utilizing inverse Compton radiation (IC) and π° decay process. Our results match well one based on IC process, as discussed in the previous papers. Those fit enable us to determine physical parameters around the shock accurately. The obtained strength of magnetic field is 4 ± 1 μG and the maximum accelerated energy in power-law distribution of the particle is Emax = 51 (B/4μG)—0.5 TeV. Energy density of the required electrons exceeds that of the magnetic field so that the system may not be in equipartition.