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.
ALMA Observes More Than Ever Before
ALMA radio telescope at night Credit: NSF/ NSF NRAO/AUI/C. Padilla
The Atacama Large Millimeter/submillimeter Array (ALMA) is thrilled to announce that a record-breaking total of 4,250 hours of science-quality data were successfully collected on the 12-m Array during Cycle 10. This surpasses the previous record of 3,787 hours achieved during Cycle 5, reflecting a significant enhancement in observational efficiency and scientific output. ALMA also set new records on its other arrays, with 3,769 hours recorded on the 7-m Array and 2,723 hours on the Total Power Array.
“This accomplishment is a direct result of the exceptional teamwork and dedication of everyone involved in the ALMA collaboration,” commented Sergio Martin, ALMA Head of the Department of Science Operations. “Achieving this level of scientific output reflects the improved operational efficiency that allows us to better cope with the growing demand for ALMA’s cutting-edge capabilities. We are excited to see the scientific discoveries emerging from the unprecedented amount of data that ALMA collects.”
This remarkable achievement is a testament to ALMA’s global team’s hard work, coordination, and dedication, including the Joint ALMA Observatory and the partner regions in East Asia, Europe, and North America. The steady increase in observing hours across recent cycles showcases ALMA’s ongoing commitment to pushing the boundaries of astronomical discovery.
This news was originally created by the Joint ALMA Observatory.
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.