By measuring the black hole mass and velocity dispersion of currently merging galaxies each in various stages of a merger, the authors conclude that the growth of the central super massive black hole occurs in the early stages of each merger and outpaces any bursts of star formation or central bulge growth.
Black holes are found in most galaxies. Observations suggest that they correlate with various properties of their host galaxies. Does this correlation hold in the very early Universe, particularly in galaxies hosting supermassive black holes? The answer is ….
What kind of lens is a BBH merger? These authors present the first pictures of light sources lensed by numerical models of BBH mergers.
Direct observational evidence for positive feedback from the interaction of outbursts from active black holes and the surrounding medium has been lacking so far, until now…
The authors report the discovery of perhaps the faintest black hole x-ray binary. But this conclusion is limited by the uncertainty in the distance to the object.
By looking at the spectral changes of the accretion disk emission around black holes, we can trace the physical changes of the accreting material.