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What a millisecond pulsar's X-ray hotspots reveal about neutron star size

Bas Dorsman, Tuomo Salmi, Anna L. Watts, Mason Ng, Anna Bobrikova, Alessandro Di Marco, Duncan K. Galloway, Sebastien Guillot, Mariska Hoogkamer, Yves Kini, Fabio La Monaca, Vladislav Loktev, Matteo Lucchini, Christian Malacaria, Ying-Han Mao, Alessandro Papitto, Juri Poutanen

May 18, 2026

Astronomers combined sharp X-ray images and polarization measurements from two space telescopes (NICER and IXPE) to map the glowing hotspots on a rapidly spinning neutron star. The pulsar's dual hotspots—one near each pole—suggest a massive, large neutron star, though many parameters sit at the edge of what the model can explain. The mismatch suggests their current picture of how these objects emit light is incomplete.
Published as Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 arXiv:2605.18731
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