Examples of using Accretion disks in English and their translations into Indonesian
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Quasars are supermassive black holes with accretion disks in the center of a galaxy.
Accretion disks around supermassive black holes are among the brightest universe objects.
In modern black holes, features called accretion disks limit the speed of growth.
The black holes are surrounded and nourished by disks of gas and dust,called accretion disks.
There simply isn't enough matter or energy in their accretion disks to create large X-ray signatures.
Neutron stars and accretion disks around black holes emit X-rays, which enable us to study them.
The latest discovery indicates that the formation of objects from accretion disks are similar for planets, brown dwarfs and stars.
Accretion disks are common around smaller stars or stellar remnants in a close binary or black holes in the centers of spiral galaxies.
In the ancient Universe, these brilliant accretion disks dazzled Spacetime in the form of quasars.
Accretion disks are often used as tools to study black holes since, unlike black holes themselves, they give off light.
Previous research suggested that the accretion disks of black holes can have dramatic effects on galaxies.
The new technology ledThorne to discover information about the gravitational lensing and accretion disks surrounding black holes.
And supermassive black holes have accretion disks that emit so much energy that astronomers can detect and even photograph them.
To capture the effects of differentblack holes we used realistic simulations of accretion disks with near-identical initial setups.
Accretion disks are common around smaller stars, or stellar remnants in a close binary, or black holes surrounded by material, such as those at the centers of galaxies.
In the ancient Universe, these brilliant accretion disks dazzled Spacetime in the form of quasars.
As such, researchers previously suggested the system's variable flickeringwas due to instabilities that can occur in accretion disks when they get very massive.
Supermassive black holes and their surrounding accretion disks can be, at least, as vast as our entire Solar System.
By measuring the energy lost from the photoionization, the researchers could measure total energy emitted from the implosion anduse it to improve their understanding of the behavior of x-rays emitted by accretion disks.
Supermassive black holes and their surrounding accretion disks can be, at least, as vast as our entire Solar System.
Accretion disks are ubiquitous features in the universe and can be found around smaller stars or stellar remnants, in close binary stars, in the centers of spiral galaxies, in quasars, they form also in gamma-ray bursts.
The reason is the underlying physics of the so called accretion disks accompanying the birth of the very first stars.
Red giants don't have accretion disks, but many most likely have companion stars, which presumably have lower masses because they are evolving more slowly.
To get the effects of black holes, realistic simulations of accretion disks with almost identical initial settings were used.
And neutron stars can also have accretion disks that produce X-rays, so astronomers must study the properties of these X-rays carefully when trying to determine what kind of object is at the center of the disk. .
For their discovery and study of the magnetorotational instability, and for demonstrating that this instability leads to turbulence andis a viable mechanism for angular momentum transport in astrophysical accretion disks.
The same process is expected to produce accretion disks around virtually all newly forming stars in the universe, some of which yield planets.
The researchers said that they were surprised to findsimilar brightness variations not only in accretion disks surrounding black holes but also in disks surrounding other celestial objects, including white dwarf stars and young stellar objects.
The same process is expected to produce accretion disks around virtually all newly forming stars in the universe, some of which yield planets.[30].