Simulations of Turbulence in Black Hole Coronae
In today’s bite, the authors use simulations to explore turbulence a possible mechanism for the observed x-ray emissions in the coronae of black holes.
In today’s bite, the authors use simulations to explore turbulence a possible mechanism for the observed x-ray emissions in the coronae of black holes.
Something is stirring up chaos on galactic scales. The authors of today’s papers investigate just what’s needed to recreate the turbulence seen in the interstellar medium.
Making a star cluster from scratch is no easy task. Today’s paper addresses the big question: what does it take to get the recipe right?
Ever wondered what role turbulence and other aspects of fluid dynamics play in the formation of stars in galaxies? Find out at Dr. Burkhart’s #AAS238 Annie Jump Cannon Prize lecture on Tuesday, 8th June!
The fractal dimension as a new way to explore the mysterious link between turbulence and star formation.
Can we teach a machine to reproduce the physics of turbulence? An exploration of using deep learning to simulate magnetohydrodynamic turbulence!