This enabled the astronomers to measure the diameter
of the accretion disc and plot its various temperatures, providing a new experimental confirmation of how quasars work.
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.
Not exact matches
The swirls within the wrap remind me greatly
of elliptical orbits
of planets, the theoretical shape
of galaxies, and even the
accretion disc of the black hole.
But now researchers from the Niels Bohr Institute have discovered a system consisting
of two stars with three rotating planet - forming
accretion discs around them.
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.
Computer simulations suggest that when two black holes spiral towards each other on a collision course, much
of the gas and dust in the spinning
accretion disc surrounding each
of them is ripped away by the gravity
of the other.
The researchers modeled the resulting
accretion disc — an elliptical
disc of stellar debris swirling around the black hole — along with its probable speed, radius, and rate
of infall, or speed at which material falls onto the black hole.
Models suggest that
accretion discs could reach the size
of a solar system and glow as brightly as a star.
About half
of the disrupted star moves in elliptical orbits around the black hole and forms an
accretion disc which eventually shines brightly in optical and X-ray wavelengths.
«If there are many axion stars in the centres, we expect that some
of them collide with the black hole
accretion disc,» says Iwazaki.
Their tendency would be to cluster near the centre
of galaxies, making them more likely to pass near the supermassive black holes that sit there and run into the
accretion discs of gas that surround them.
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.
The sun formed at the hot and dense centre
of this
disc, while the planets grew by
accretion in the cooler outer regions.
Those would cluster near the centre
of galaxies, making them more likely to pass through the
accretion discs of supermassive black holes there, causing the bursts we detect.
Kip Thorne worked out the mathematics
of what happens to the
accretion disc, and found that the intense gravity warps the
disc around the black hole, creating the spectacular halo that is one
of the movie's visual highlights.
They discuss a unified scenario for understanding brightness variations from
accretion discs around different types
of stars and compact objects.
At the presentations
of their research results, the two students showed their findings respectively focused on (i)
Accretion and rotational movement
of gas around a protostar and the formation
of a circumstellar
disc and (ii) Identification
of bipolar jets (mass ejection) from multiple protostars and classification according to the evolutionary phases.