New radio images from the the U.S. National Science Foundation Very Large Array trace a pair of powerful plasma jets launched by galaxy VV 340a’s central supermassive black hole, which appear to be driving hot coronal gas out of the galaxy and shutting down future star formation.
Recent News
Radio Telescopes Uncover ‘Invisible’ Gas Around Record-Shattering Cosmic Explosion
Astronomers using the U.S. National Science Foundation Very Large Array and the Atacama Large Millimeter/submillimeter Array have revealed a dense cocoon of gas around one of the most extreme cosmic explosions ever seen, showing that a ravenous black hole ripped apart a massive star and then lit up its surroundings with powerful X-rays.
New Discovery Challenges Evolution of Galaxy Clusters
Peering back in time, around 12 billion years, astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have found the most distant and direct evidence of scorching gas in a forming galaxy cluster, SPT2349-56. The hot plasma, seen when the Universe was just 1.4 billion years old, is far hotter and more pressurized than current theories predicted for such an early system.
New type of Fast Radio Burst discovered in Green Bank Telescope data
Artist’s impression of the discovery of microsecond Fast Radio Bursts being observed by the Green Bank Telescope. Incoming radio waves are shown as white, red, and orange streaks that follow each other in rapid succession. The long red streaks are the previously known millisecond flashes. (c) Daniëlle Futselaar/www.artsource.nl
An international team of researchers have discovered radio pulses from the distant universe that last only millionths of a second. They found these microsecond bursts after a meticulous examination of archival data from the National Science Foundation’s Green Bank Telescope. It’s unclear how the ultrafast bursts were created. The researchers published their findings in Nature Astronomy.
Fast radio bursts (FRBs) are unpredictable, extremely short flashes of radio waves far beyond our Milky Way. They are possibly caused by magnetic neutron stars, also known as magnetars. The first bursts were discovered in 2007. So far, most bursts last longer than a thousandth of a second and emit as much energy as our sun generates in a day.
In 2022, researchers at the University of Amsterdam and ASTRON hypothesized that there might be bursts that would last not thousandths, but only millionths of a second. “During our group meetings, we often talked about it”, says Mark Snelders, PhD candidate at ASTRON and the University of Amsterdam (the Netherlands), who was in charge of the research that uncovered the ultra-fast radio bursts. “By coincidence, I found out that there was a public dataset that we could use for this.”
Watch a presentation by Mark for the Green Bank Observatory about this science.
Five hours of data – and millions of images
The researchers accessed the public data archive from the Breakthrough Listen project, which uses the Green Bank Telescope to search for extraterrestrial life. They focused on five hours of data from FRB 20121102A, located some three billion light years away, towards the Auriga constellation.
The researchers divided each second of the first thirty minutes of data into half a million individual images. Next, they used software filters and machine learning to search for outliers. Through this meticulous process, they discovered eight ultra-fast bursts that lasted only ten millionths of a second or less.
Now that the first ultra-fast microsecond source has been detected, researchers expect to find more. However, finding them may be easier said than done, as some data files are not detailed enough to cut into half a million pieces per second.
The Green Bank Observatory is supported by the National Science Foundation and is operated by Associated Universities, Inc.
Read more at the Netherlands Research School for Astronomy.
Media Contact:
Jill Malusky, NRAO & GBO News & Public Information Manager
[email protected]
This news article was originally published on the GBO website on October 19, 2023.
Recent News
The NSF Very Large Array Helps Reveal Record-Breaking Stream of Super-Heated Gas from Nearby Galaxy
New radio images from the the U.S. National Science Foundation Very Large Array trace a pair of powerful plasma jets launched by galaxy VV 340a’s central supermassive black hole, which appear to be driving hot coronal gas out of the galaxy and shutting down future star formation.
Radio Telescopes Uncover ‘Invisible’ Gas Around Record-Shattering Cosmic Explosion
Astronomers using the U.S. National Science Foundation Very Large Array and the Atacama Large Millimeter/submillimeter Array have revealed a dense cocoon of gas around one of the most extreme cosmic explosions ever seen, showing that a ravenous black hole ripped apart a massive star and then lit up its surroundings with powerful X-rays.
New Discovery Challenges Evolution of Galaxy Clusters
Peering back in time, around 12 billion years, astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have found the most distant and direct evidence of scorching gas in a forming galaxy cluster, SPT2349-56. The hot plasma, seen when the Universe was just 1.4 billion years old, is far hotter and more pressurized than current theories predicted for such an early system.