A gigantic new interpretation shows the moment a cosmic giant swallows a star.
Because of the tearing of this star, astronomers call it the ‘oscillating phenomenon’, which is accompanied by the emission of radiation that can exceed the combined light of each star in the host galaxy for several months or even years.
This particular black hole was captured using X-rays emitted from a tidal wave phenomenon called J2150, which is a type-an intermediate-mass black hole except for a long-term observation.
“We were able to capture this black hole that swallows a star, which provides a wonderful opportunity to observe what is otherwise invisible,” said Ann Jablotoff, co-author of the paper and a professor at the University of Arizona. We were able to understand this elusive class of black holes that are responsible for most of the black holes in the center of the galaxy.
By reviewing the X-ray data used to observe the J2150 light and comparing it to complex theoretical models, the researchers showed that the glow actually appeared from the junction between a star and a medium-mass black hole.
The team was able to classify it as an intermediate black hole after measuring its mass and rotation, said Sixiang Wen, a postgraduate researcher at the Stewart Laboratory at the University of Arizona.
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Dozens of wave disturbances have been observed at the centers of large galaxies that hold miraculous black holes, and a few at the centers of smaller galaxies with intermediate black holes.
However, previous data have not been sufficiently detailed to prove that a single wave of chaos erupted by an intermediate black hole.
Nicholas Stone, co-author of the study, a lecturer at the Hebrew University, said: “Thanks to recent astronomical observations, we know that the centers of almost all galaxies resemble our Milky Way galaxy or very large black holes.”
These giant planets are 1 million to 10 billion times larger than our Sun, and become powerful sources of electromagnetic radiation when more galaxy gas falls near them.
The mass of these black holes is closely related to the total mass of their host galaxies, so the largest galaxies have the largest marvelous black holes.
“We know very little about the presence of black holes in the centers of galaxies smaller than the Milky Way,” said Peter Junker, an associate professor at the University of Rodbout in the Netherlands.
Due to observation limitations, it is difficult to detect very small central black holes larger than 1 million solar masses.
Although black holes are thought to be abundant, the origin of high-velocity black holes is unknown.
One theory, however, is that medium-mass black holes may be the seeds from which miraculous black holes grow.
“Once we get a better handle on how many intermediate black holes there are, it will help determine the exact principles for creating supermassive black holes,” Junker added.
Spiral measurements allow astronomers to test hypotheses about the nature of dark matter, which is believed to form most objects in the universe.
Dark matter may contain elemental particles that have not yet been found in laboratory tests.
In the future, new observations of ripple radiation will allow astronomers to fill in the blanks regarding the distribution of certain types of black holes.
New telescopes on Earth and in space are expected to detect thousands of tidal events each year.
Source: Daily Mail
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