Gamma-ray pulsations reveal extreme 3.2-millisecond pulsar 3,900 light-years away

Astronomers using NASA's Fermi gamma-ray space telescope have identified gamma-ray pulsations from a millisecond pulsar, PSR J0435+3233. Located 3,900 light-years away, this binary system exhibits extreme spin-down luminosity, making it a significant subject for astrophysical study.
Why it matters
Understanding the properties of extreme pulsars helps scientists refine models of neutron star evolution and binary system dynamics.
edited by Sadie Harley , reviewed by Robert Egan
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Add as preferred source Test statistic (TS) maps of the 5◦ ×5◦ region centered on PSR J0435+3233 in the 0.1–500.0 GeV, constructed using events collected within the ephemeris-valid interval (EVI). Left and right panels show the on-pulse and off-pulse TS maps, respectively. Credit: Zhang et al., 2026. By analyzing the data from NASA's Fermi gamma-ray space telescope, Chinese astronomers have investigated a recently identified millisecond pulsar known as PSR J0435+3233. As a result, they found that the pulsar exhibits gamma-ray pulsations. The discovery was detailed in a paper published July 17 on the pre-print server arXiv .
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