A pair of supermassive black holes has been found consuming an enormous gas cloud, unlike anything seen before. The discovery, made possible by a peculiar radiation signal, provides insight into the behavior of supermassive black holes and their relationship with the galaxies they inhabit.
The signal was first detected in March 2021 in a galaxy located approximately 1 billion light-years away, in the northern constellation Cygnus. Scientists suspected the signal might be linked to supernovas or tidal disruption events but a highly unusual oscillation pattern warned this was not that case.
Observations with a range of wavelengths confirmed that the signal's origin was unfamiliar. The researchers turned to theoretical models to solve the mystery. They hypothesized that the radiation was produced by a pair of supermassive black holes consuming a massive cloud of galactic gas.
Based on the simulation, the light emitted by the system can be explained by a binary supermassive black hole interacting with a gas cloud roughly equivalent in mass to the Sun. The two black holes are separated by 0.8 milliparsecs, orbit each other roughly every 130 days, have a combined mass of about 40 million solar masses, and are expected to merge in approximately 70,000 years.
If validated, this discovery could transform how astronomers study supermassive black holes by offering a new method to investigate their evolution and their role in shaping galaxies.
These massive objects are closely linked to their host galaxies, and learning more about their feeding habits could provide fresh insight into galactic development.
Finding binary supermassive black holes is a challenging task, but it is expected to be present in many galaxy centers.
The fact that we cannot resolve the two black holes with the available instrumentation implies that we need to find alternative techniques to detect them through other methods.
Additional observations of similar systems will be necessary to solidify their conclusions. Future data will help refine models of how supermassive black holes behave when consuming galactic gas.
New data and simulations using these data are required to confirm the scenario that they are proposing to probe the authors' hypothesis.