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.
Modelling for National Security
AUI Joins BEACONS Center and LEAP Manufacturing Efforts
AUI has joined with LEAP Manufacturing in support of the UT Dallas Batteries and Energy to Advance Commercialization and National Security (BEACONS) Center, which will develop and commercialize new battery technologies and manufacturing processes, enhance the domestic availability of critical raw materials, and train high-quality workers for jobs in an expanding battery energy storage workforce. BEACONS is funded by a $30M agreement over three years by the U.S. Department of Defense. AUI’s role will relate to modelling the critical mineral supply chain.
Enhancing the domestic manufacturing of batteries for commercialization and national security needs requires a better understanding of the critical material supply chain and efforts to support Defense contractors’ ability to produce batteries domestically. UT Dallas and LEAP Manufacturing are positioning BEACONS to guide the optimization of existing battery systems, foster new battery chemistries, identify and track supply chain challenges, and promote workforce development.
Tom Campbell, Co-Director of LEAP Manufacturing emphasized “the need for exploring advanced manufacturing for the battery supply chain, including related critical materials, is a national need, and BEACONS will help address the gaps.”
“Better, more informed decision making starts with the supply chain,” AUI President Adam Cohen said. “It’s exciting to be part of the battery campus, which will help identify and pursue battery chemistries and manufacturing capabilities that will be important for the country’s economic and national security.”
AUI is an independent, not-for-profit founded in 1946 that specializes in the design, construction, and management and operations of cutting-edge research facilities and development and implementation of innovative approaches to education, outreach and workforce development. AUI manages the National Radio Astronomy Observatory (NRAO) and the Green Bank Observatory (GBO) for the National Science Foundation (NSF).
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.