Мақаланы E-mail арқылы жіберу Acceleration of particles and generation of nonthermal emission in old supernova remnants
- Авторлар: Zirakashvili V.N.1, Ptuskin V.S.1
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Мекемелер:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN)
- Шығарылым: Том 81, № 4 (2017)
- Беттер: 434-436
- Бөлім: 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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Аннотация
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.
Авторлар туралы
V. Zirakashvili
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN)
Хат алмасуға жауапты Автор.
Email: zirak@izmiran.ru
Ресей, Troitsk, Moscow, 108840
V. Ptuskin
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN)
Email: zirak@izmiran.ru
Ресей, Troitsk, Moscow, 108840
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