Ten high school students have been awarded for academic achievement, community involvement and leadership skills.
ALMA and the Event Horizon Telescope: Moving Towards a Close-Up of a Black Hole and its Jets
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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.
ALMA and the Event Horizon Telescope: Moving Towards a Close-Up of a Black Hole and its Jets
Credit: Chalmers/J. Bournonville/Anne-Kathrin Baczko
After taking the first images of black holes, the ground-breaking Event Horizon Telescope (EHT) is poised to reveal how black holes launch powerful jets into space. An international research team has shown that the EHT will be able to make exciting images of a supermassive black hole and its jets in the galaxy NGC 1052. The measurements, made with interconnected radio telescopes, also confirm strong magnetic fields close to the black hole’s edge.
“The centre of this galaxy, NGC 1052, is a promising target for imaging with the Event Horizon Telescope, but it’s faint, complex and more challenging than all other sources we’ve attempted so far”, says Anne-Kathrin Baczko, an astronomer at Onsala Space Observatory, Chalmers and the lead of this research.
The team made measurements using just five of the telescopes in the EHT’s global network – including ALMA, including ALMA (the Atacama Large Millimeter/submillimeter Array), of which the U.S. National Science Foundation National Radio Astronomy Observatory is a partner, in a configuration that would allow the best possible estimate of its potential for future observations, and supplemented with measurements from other telescopes.
“For such a faint and unknown target, we were not sure if we would get any data at all. But the strategy worked, thanks in particular to the sensitivity of ALMA and complementary data from many other telescopes”, says Anne-Kathrin Baczko.
This text was adapted from a press release shared by Chalmers University. View the full release.
This news article was originally published on the NRAO website on December 17, 2024.
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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.