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.
Today’s bite delves into the tragic final encounter between a supermassive black hole and its stellar neighbour that came a bit too close.
Neutron stars (NSs) are the most extreme objects known, composed of a form of matter so extraordinarily dense that it teeters on the brink of collapse into a black hole.
Everyone wants to find a habitable planet. The authors of today’s paper make a compelling case that the HR 5183 system is not the best place to look.
Pulsar timing arrays could localise individual sources of gravitational waves to host galaxies. The problem is, it’s so computationally difficult! This paper shows us a faster way.
Today’s paper looks at the impact of AGN feedback on X-ray emission around an unprecedented sample of galaxy groups!