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Simons Collaboration on Extreme Electrodynamics of Compact Sources
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linkhttps://www.simonsceecs.com/ calendar_today01-04-2024 17:47:21

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2 years ago

Groselj et al. use PIC simulations of strong electromagnetic turbulence as a possible mechanism for explaining observed X-ray emission from black hole coronae, specifically comparing predictions with Cygnus X-1. Read here: astrobites.org/2024/03/23/tur…

Groselj et al. use PIC simulations of strong electromagnetic turbulence as a possible mechanism for explaining observed X-ray emission from black hole coronae, specifically comparing predictions with Cygnus X-1. Read here: astrobites.org/2024/03/23/tur…