November 10, 2021 report
Data from the Fermi Large Area Telescope suggests there is a particle accelerator in the galactic center
A team of researchers at the Chinese Academy of Sciences has found evidence of a powerful particle accelerator in the galactic center. In their paper published in the journal Nature Communications, the group describes their analysis of data obtained from the Fermi Large Area Telescope.
The galactic center is the rotational center of the Milky Way galaxy—prior research has shown that it contains a large black hole. There are also other entities in the galactic center, such as remnants from supernovae and the pulsar wind nebulae, but not much else is known about the interior of the galactic center due to its density. The cloud is so thick that it is nearly impossible to read many of the forms of radiation within it. Still, most in the field agree that the galactic center emits a lot of cosmic rays, many of which could be important because they make it to Earth.
In this new effort, the researchers sought to learn more about the cosmic rays emitted from the galactic center, particularly those that make their way to Earth. To that end, they obtained and analyzed data collected by various teams working at the Fermi Large Area Telescope. They focused most specifically on gamma rays emitted from the central molecular cloud—a type of cloud that forms from interstellar dust and hydrogen gas—situated between Earth and the galactic center. They found that the density of cosmic rays in the central molecular cloud was lower than that in the cosmic ray sea, which suggested that there is a barrier of some sort preventing cosmic rays from entering the central molecular cloud. But they also found evidence of the cosmic rays slowing as they passed through the cloud and then speeding up again after they emerged—evidence that something near the center of the galaxy serves as a particle accelerator. They were not able to find evidence of what it might be, but suspect it could be the black hole, Sagittarius A*, wind nebulae or even leftover bits of a supernova.
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