Known
as an accretion disc, it is the place where material gradually spirals inwards towards the black hole.
Not exact matches
The study found a relationship between the size of the central object and the speed of the flickering produced by the
disc, suggesting the physics of the
accretion must be very similar around these different astronomical objects despite them being completely different in other ways, such
as size, age, temperature and gravity.
The researchers found that relatively cool
accretion discs around young stars, whose inner edges can be several times the size of the Sun, show the same behaviour
as the hot, violent
accretion discs around planet - sized white dwarfs, city - sized black holes and supermassive black holes
as large
as the entire Solar system, supporting the universality of
accretion physics.
Models suggest that
accretion discs could reach the size of a solar system and glow
as brightly
as a star.
Such
discs, known
as quasar
accretion disks, are typically about 100 billion kilometers across, and most lay billions of light - years away.
So if astronomers can understand the physics of the matter that is flowing into the black hole, they can use it to test the predictions of general relativity
as never before — but only if the movement of the matter in the
accretion disc can be completely understood.
We interpret this periodicity
as a property of the
accretion disc, most likely a long - term precession, where the
disc edge structure and X-ray irradiation is responsible for the hard X-ray dips and modulation, although we discuss other possible explanations, including Lense - Thirring precession in the inner
disc region and spectral state variations.