A new study connects the black hole’s famous ring of light to a compact region that marks the likely base of the jet, bringing scientists closer to understanding how black holes power some of the brightest beacons in the universe.
Recent News
Magnetic Superhighways Discovered in a Starburst Galaxy’s Winds
Using the Atacama Large Millimeter/submillimeter Array (ALMA), an international team of astronomers has mapped a magnetic highway driving a powerful galactic wind into the nearby galaxy merger of Arp 220, revealing for the first time that its fast, molecular outflows are strongly magnetized and likely helping to drive metals, dust, and cosmic rays into the space around the galaxy.
Making Scientific Breakthroughs Possible in 2025
2025 was an incredibly productive year for AUI, marked by significant advances across astronomy, energy, advanced therapeutics, and STEM education and workforce development.
IMAGE RELEASE: Galaxies in the Perseus Cluster
For galaxies, as for people, living in a crowd is different from living alone. Recently, astronomers used the National Science Foundation’s Karl G. Jansky Very Large Array (VLA) to learn how a crowded environment affects galaxies in the Perseus Cluster, a collection of thousands of galaxies some 240 million light-years from Earth.
Left: The giant galaxy NGC 1275, at the core of the cluster, is seen in new detail, including a newly-revealed wealth of complex, filamentary structure in its radio lobes.
Center: The galaxy NGC 1265 shows the effects of its motion through the tenuous material between the galaxies. Its radio jets are bent backward by that interaction, then merge into a single, broad “tail.” The tail then is further bent, possibly by motions within the intergalactic material.
Right: The jets of the galaxy IC 310 are bent backward, similarly to NGC 1265, but appear closer because of the viewing angle from Earth. That angle also allows astronomers to directly observe energetic gamma rays generated near the supermassive black hole at the galaxy’s core.
Such images can help astronomers better understand the complex environment of galaxy clusters, which are the largest gravitationally-bound structures in the universe, and which harbor a variety of still poorly-understood phenomena.
“These images show us previously-unseen structures and details and that helps our effort to determine the nature of these objects,” said Marie-Lou Gendron-Marsolais, an ESO/ALMA Fellow in Santiago, Chile. She and a number of international collaborators are announcing their results in the Monthly Notices of the Royal Astronomical Society.
The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.
CREDIT: M. Gendron-Marsolais et al.; S. Dagnello, NRAO/AUI/NSF; SDSS.
###
Media Contact:
Dave Finley, Public Information Officer
(575) 835-7302
[email protected]
###
This news article was originally published on the NRAO website on November 12, 2020.
Recent News
New Event Horizon Telescope Results Trace M87 Jet Back to Its Black Hole
A new study connects the black hole’s famous ring of light to a compact region that marks the likely base of the jet, bringing scientists closer to understanding how black holes power some of the brightest beacons in the universe.
Magnetic Superhighways Discovered in a Starburst Galaxy’s Winds
Using the Atacama Large Millimeter/submillimeter Array (ALMA), an international team of astronomers has mapped a magnetic highway driving a powerful galactic wind into the nearby galaxy merger of Arp 220, revealing for the first time that its fast, molecular outflows are strongly magnetized and likely helping to drive metals, dust, and cosmic rays into the space around the galaxy.
Making Scientific Breakthroughs Possible in 2025
2025 was an incredibly productive year for AUI, marked by significant advances across astronomy, energy, advanced therapeutics, and STEM education and workforce development.