Birth of a Magnetar Captured Inside a Brilliant Supernova

TL;DR Summary
Astronomers have for the first time witnessed the birth of a magnetar—an ultra-strongly magnetized neutron star—at the heart of a rare, superluminous supernova (SN 2024afav). The event’s peculiar light curve, including four diminishing “chirps” caused by a Lense–Thirring precession of a disk around the newborn magnetar, provides the first observational link between such births and magnetar-powered superluminous explosions, with the object estimated to spin ~4.2 milliseconds and harbor a magnetic field about 300 trillion times Earth's.
- Scientists witness birth of one of the universe's strongest magnets for the first time, thanks to a general relativity 'magic trick' Live Science
- Astronomers witness colossal supernova explosion create one of the most magnetic stars in the universe for the first time Space
- Lense–Thirring precessing magnetar engine drives a superluminous supernova Nature
- UCSB researcher bridges the worlds of general relativity and supernova astrophysics UC Santa Barbara
- Spinning Magnetar (IMAGE) EurekAlert!
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