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Researchers have discovered that a bright, pulsing neutron star is the source of ultra-bright X-rays coming from near the centre of the nearby galaxy Messier 82.

Researchers have previously thought that only a black hole could emit so brightly in the X-ray region, but the team found that the source was pulsing, which black holes cannot do.

This discovery that neutron stars can emit such high X-ray luminosities suggests that the physics within neutron stars are even more extreme than what was thought possible.

Original research paper published in Nature on October 8, 2014.

Names and affiliations of selected authors

Matteo Bachetti, Université de Toulouse, France

Victoria Kaspi, McGill University, Quebec