Optical and ultraviolet pulsed emission from an accreting millisecond pulsar

Millisecond spinning, low-magnetic-field neutron stars are believed to attain their fast rotation in a 0.1–1-Gyr-long phase during which they accrete matter endowed with angular momentum from a low-mass companion star 1 . Despite extensive searches, coherent periodicities originating from accreting neutron star magnetospheres have been detected only at X-ray energies 2 and in ~10% of the currently known systems 3 . Here we report the detection of optical and ultraviolet coherent pulsations at the X-ray period of the transient low-mass X-ray binary system SAX J1808.4−3658, during an accretion outburst that occurred in August 2019 4 . At the time of the observations, the pulsar was surrounded by an accretion disk, displayed X-ray pulsations and its luminosity was consistent with magnetically funnelled accretion onto the neutron star. Current accretion models fail to account for the luminosity of both optical and ultraviolet pulsations; these are instead more likely to be driven by synchro-curvature radiation 5 , 6 in the pulsar magnetosphere or just outside of it. This interpretation would imply that particle acceleration can take place even when mass accretion is going on, and opens up new perspectives in the study of coherent optical/ultraviolet pulsations from fast-spinning accreting neutron stars in low-mass X-ray binary systems. Outbursts from accreting pulsars encode much information on mass accretion in X-ray binary systems. Measuring optical as well as X-ray pulsations can constrain models and, indeed, point to particle acceleration taking place during accretion.