New Chandra observations of 4U 0114+65 reveal pulse-to-pulse brightness cycles that the authors attribute to repeated accumulation and depletion of matter at the neutron star's magnetosphere.
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Cyclical accretion regime change in the slow X-ray pulsar 4U 0114+65 observed with Chandra
New Chandra observations of 4U 0114+65 reveal pulse-to-pulse brightness cycles that the authors attribute to repeated accumulation and depletion of matter at the neutron star's magnetosphere.