电邮这篇文章 Acceleration of particles and generation of nonthermal emission in old supernova remnants
- 作者: Zirakashvili V.N.1, Ptuskin V.S.1
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隶属关系:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN)
- 期: 卷 81, 编号 4 (2017)
- 页面: 434-436
- 栏目: Proceedings of the 34th National Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/185034
- DOI: https://doi.org/10.3103/S1062873817040426
- ID: 185034
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详细
Particle acceleration by shock waves in old supernova remnants is studied. The radiative loss of gas behind the front of a shock wave, the streaming instability of magnetohydrodynamic waves, and the damping of waves on neutral atoms are considered. The calculated spectra of electromagnetic emissions are compared to observations of supernova remnant IC 443.
作者简介
V. Zirakashvili
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN)
编辑信件的主要联系方式.
Email: zirak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 108840
V. Ptuskin
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN)
Email: zirak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 108840
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