Fermi Bubbles Explained: Fast Outward Winds and ‘Reverse Shock’ at Center of Galaxy
Updated: 2022-12-31 14:40:16
: Skip to content Menu Our Bloggers Twitter Google News Substack FaceBook Contribute Contact Search Fermi Bubbles Explained : Fast Outward Winds and Reverse Shock’ at Center of Galaxy December 31, 2022 Tokyo Metropolitan University Summary Fast winds blowing outward from the center of the Milky Way might have created the large , gamma-ray emitting Fermi bubbles” found around the center of our galaxy . Researchers used simulations and measurements from an X-ray telescope to support this idea . The winds predicted by the simulation are similar to outflows observed in other galaxies , which suggests that similar winds may have been present in our own galaxy until . recently A scientist from Tokyo Metropolitan University has shown that large gamma-ray emitting bubbles around the center of our