. | . |
Gamma ray discovery could advance understanding of ultra-fast outflows by Staff Writers Stanford CA (SPX) Nov 11, 2021
Using data gathered by the Large Area Telescope onboard NASA's Fermi Gamma-ray Space Telescope and a stacking technique combining signals too weak to be observed on their own, researchers detected gamma rays from UFOs in several nearby galaxies for the first time, providing a basis for scientists to understand what happened in our own Milky Way galaxy. UFOs are ultra-fast outflows - powerful winds launched from very near supermassive black holes that scientists believe play an important role in regulating the growth of the black hole itself and its host galaxy. Clemson University scientists' collaborative research is published in The Astrophysical Journal. Partners include the College of Charleston, the University of Chicago, and a host of other researchers who are part of the Fermi-LAT Collaboration, which includes hundreds of scientists from 12 countries. "Gamma rays from Fast Black-Hole Winds" outlines the detection of gamma-ray emission from UFOs launched by supermassive black holes. "Although these winds are challenging to detect, it is thought that they play a significant role in how a massive black hole and the host galaxy itself grow," said Chris Karwin, a postdoctoral fellow in the College of Science's Department of Physics and Astronomy and leader of the study. "Our gamma-ray observations show how supermassive black holes can transfer a large amount of energy to their host galaxy. These UFOs create shock waves, which act like pistons and actually accelerate charged particles, known as cosmic rays, to near the speed of light." Every galaxy has a supermassive black hole at its center. Some are dormant. Others, called active galactic nuclei, are active, meaning that they draw in and "eat" the surrounding matter through a process called accretion. While traveling through the galaxies, the winds gradually disable star formation. "The effect on the galaxy is dramatic," Ajello said. "The black hole at the center of the galaxy and the galaxy itself have a mechanism to grow together in mass - and this is the mechanism." Because the gamma rays detected are produced by cosmic rays accelerated at the shock front, Karwin said it attests to the onset of the wind-host interaction and that the UFOs can energize charged particles up to the transition region between galactic and extragalactic cosmic rays.
Understanding the Milky Way Sagittarius A* is the supermassive black hole at the center of the Milky Way with about 4 million times the sun's mass. Extending above and below the Milky Way's disc are Fermi bubbles, enormous round structures of hot gas emanating from the galactic center. They're called Fermi bubbles because the Fermi Gamma-Ray Space Telescope, the source of the data used by Ajello and Karwin in the current study, discovered them in 2010. "Today, our black hole, Sagittarius A*, is not active, but it's possible it was active in the recent past, maybe up until a few hundred years ago," Karwin said. "Our model supports the hypothesis that these Fermi bubbles may be remnants of past UFO-like activity from the supermassive black hole in the center of our galaxy." Ajello said future work includes studying galaxies that have had active UFO winds for 10s of millions of years that have already traveled to the outskirts of the galaxy.
NASA's Fermi Spots a Supernova's 'Fizzled' Gamma-ray Burst Greenbelt MD (SPX) Jul 27, 2021 On Aug. 26, 2020, NASA's Fermi Gamma-ray Space Telescope detected a pulse of high-energy radiation that had been racing toward Earth for nearly half the present age of the universe. Lasting only about a second, it turned out to be one for the record books - the shortest gamma-ray burst (GRB) caused by the death of a massive star ever seen. GRBs are the most powerful events in the universe, detectable across billions of light-years. Astronomers classify them as long ... read more
|
|
The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us. |