PSR B0943+10 is a pulsar, which is a highly magnetized, rotating neutron star that emits a beam of electromagnetic radiation. As the neutron star rotates, this beam can be observed from Earth as it sweeps across our line of sight, producing a series of pulses, typically in the radio wavelength. Discovered in 1968, PSR B0943+10 is notable within the pulsar community for several reasons.
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