Shock Waves in the Magnetic Reconnection in the Flares on the Accretion Disk of the Sgr A*
Sgr A* often shows bright, episodic flares observationally, but the mechanism of the flares' intermittent brightening is not very clear. Many people believe the flares may be formed by the nonthermal particles, which can be a consequence of the magnetic reconnection and shock waves. In this wor...
| الحاوية / القاعدة: | The Astrophysical Journal |
|---|---|
| المؤلفون الرئيسيون: | , , , |
| التنسيق: | مقال |
| اللغة: | الإنجليزية |
| منشور في: |
IOP Publishing
2024-01-01
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| الموضوعات: | |
| الوصول للمادة أونلاين: | https://doi.org/10.3847/1538-4357/ad5d58 |