In today’s astrobite we explore a new approach that has been developed to measure the Universal expansion rate, involving gravitational waves from merging black holes and the large-scale structure of the Universe.
How are the masses of growing black holes in the early universe are correlated with properties of their host galaxies? Read on to see what today’s authors found!
In today’s Astrobite, we revisit the possibility of binary black hole mergers in AGN disks creating flares, which could have interesting implications for multimessenger astronomy and cosmology.
Mass transfer is a fundamental parameter for determining how binary stars evolve. A 3D hydrodynamic simulation enables real-time movies of how material moves from one star to another!
What kind of event is violent enough to fling around stars that are hundreds of times more massive than our Sun? Find out today!
Some astronomers are discovering black holes that appear to be too big for their galaxies. Discover how rapid growth could be the cause!