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| Illustration Credit: NASA courtesy of IXPE team |
Some of the brightest objects in the sky are called blazars. They consist of a supermassive black hole feeding off material swirling around it in a disk, which can create two powerful jets perpendicular to the disk on each side. A blazar is especially bright because one of its powerful jets of high-speed particles points straight at Earth. For decades, scientists have wondered: How do particles in these jets get accelerated to such high energies?
NASA’s Imaging X-Ray Polarimetry Explorer, or IXPE, has helped astronomers get closer to an answer. In a new study in the journal Nature, authored by a large international collaboration, astronomers find that the best explanation for the particle acceleration is a shock wave within the jet.
Manel Errando, an assistant professor of physics in Arts & Sciences at Washington University in St. Louis, and a faculty fellow of the McDonnell Center for the Space Sciences, is part of the team that analyzed the IXPE data.
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