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• W2030087079 abstract "The ROSAT HRI was used to monitor X-ray emission from the Vela pulsar. Six observations span 2.5 yr and three glitches. The summed data yield a determination of the pulse shape, and X-ray emission from the pulsar is found to be 12% pulsed with one broad and two narrow peaks. One observation occurred 15 days after a large glitch. No change in pulse structure was observed, and any change in X-ray luminosity, if present, was less than 3%. Implications for neutron star structure are discussed." @default.
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• W2030087079 date "2000-06-20" @default.
• W2030087079 modified "2023-10-17" @default.
• W2030087079 title "ROSATObservations of the Vela Pulsar" @default.
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• W2030087079 doi "https://doi.org/10.1086/308961" @default.
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