The proposed array’s design will improve on the sensitivity and spatial resolution—with 10 times the effective collecting area and resolution—over the current NSF VLA and the Atacama Large Millimeter/submillimeter Array at the same wavelengths.
The NSF Very Large Array Helps Reveal Record-Breaking Stream of Super-Heated Gas from Nearby Galaxy
Recent News
VLBA Maps Turbulent ‘Weather’ in the Milky Way
Astronomers using the U.S. National Science Foundation’s Very Long Baseline Array (NSF VLBA), operated by the NSF National Radio Astronomy Observatory (NSF NRAO), have made the first clear, radio-wavelength detection of how turbulent gas in our own Galaxy distorts light from a distant quasar.
Painting the Giant: NSF Green Bank Telescope Gets Critical Makeover
This work is part of a multi-year repainting effort designed to protect this national scientific asset from the elements and extend the NSF GBT’s working life for future generations of researchers.
The NSF Very Large Array Helps Reveal Record-Breaking Stream of Super-Heated Gas from Nearby Galaxy
Astronomers using the U.S. National Science Foundation Very Large Array (NSF VLA), together with the NASA James Webb Space Telescope and other observatories, have identified an enormous, galaxy-scale stream of super-heated gas erupting from the nearby galaxy VV 340a. New radio images from the NSF VLA trace a pair of powerful plasma jets launched by the galaxy’s central supermassive black hole, which appear to be driving hot coronal gas out of the galaxy and shutting down future star formation.
VV 340a lies relatively close in cosmic terms, giving astronomers an unprecedented, multiwavelength look at how radio jets from a feeding black hole can carve through a galaxy’s disk, stir up its gas, and limit its ability to grow new stars. In VV 340a, the jets extend on kiloparsec scales and follow a helical path, clear evidence that they slowly change direction over time in a process known as jet precession. This is the first time astronomers have seen a precessing, kiloparsec-scale radio jet in a disk galaxy driving such a massive, coherent outflow of coronal gas.
Operated by the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) the NSF VLA is one of the world’s most versatile and powerful radio observatories and was essential for revealing the structure and impact of VV 340a’s jets. This result was presented on Thursday, January 8, 2026 at the 247th American Astronomical Society Conference. Read the full press release.
About NRAO
The National Radio Astronomy Observatory is a facility of the U.S. National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.
Media Contact:
Corrina C. Jaramillo Feldman
Sr. Public Information Officer
VLA, VLBA, ngVLA
[email protected]
(505) 366-7267
This news article was originally published on the NRAO website on January 8, 2026.
Recent News
NSF NRAO Leads Future of U.S. Radio Astronomy with First Light from Next Generation Very Large Array Prototype
The proposed array’s design will improve on the sensitivity and spatial resolution—with 10 times the effective collecting area and resolution—over the current NSF VLA and the Atacama Large Millimeter/submillimeter Array at the same wavelengths.
VLBA Maps Turbulent ‘Weather’ in the Milky Way
Astronomers using the U.S. National Science Foundation’s Very Long Baseline Array (NSF VLBA), operated by the NSF National Radio Astronomy Observatory (NSF NRAO), have made the first clear, radio-wavelength detection of how turbulent gas in our own Galaxy distorts light from a distant quasar.
Painting the Giant: NSF Green Bank Telescope Gets Critical Makeover
This work is part of a multi-year repainting effort designed to protect this national scientific asset from the elements and extend the NSF GBT’s working life for future generations of researchers.