An international team of researchers has detected significant X-ray oscillations near the innermost orbit of a supermassive black hole.
The extreme supermassive black hole 1ES 1927+654, located 270 million light years away, displayed rapid X-ray variability and underwent a period of undetectability for about a month before becoming the brightest supermassive black hole in the X-ray sky.
The period of the oscillations rapidly changed from around 18 minutes in 2022 to around seven minutes in 2024, which is an unprecedented finding among similar supermassive black holes.
The study suggests that the rapid X-ray period change could be driven by a white dwarf orbiting close to the supermassive black hole, raising the possibility of detecting gravitational wave signals in future.