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Swings between rotation and accretion power in a binary millisecond pulsar
DOI: 10.1038/nature12470 Bibcode: 2013Natur.501..517P

Wieringa, M. H.; Campana, S.; Stella, L. +20 more

It is thought that neutron stars in low-mass binary systems can accrete matter and angular momentum from the companion star and be spun-up to millisecond rotational periods. During the accretion stage, the system is called a low-mass X-ray binary, and bright X-ray emission is observed. When the rate of mass transfer decreases in the later evolutio…

2013 Nature
XMM-Newton INTEGRAL 412