The Physical Origin and Time Lag of Multifrequency Flares from Sgr A*
Sagittarius A*, the supermassive black hole at the center of our galaxy, exhibits flares across various wavelengths, yet its origin remains elusive. We performed 3D two-temperature general relativistic magnetohydrodynamic simulations of magnetized accretion flows initialized from multiloop magnetic...
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| Hlavní autoři: | , , , , , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
IOP Publishing
2025-01-01
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| Edice: | The Astrophysical Journal |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/1538-4357/adf1e5 |
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