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• W2754366346 abstract "Observations obtained in the last years challenged the widespread notion that rotation-powered neutron stars are steady X-ray emitters. Besides a few allegedly rotation-powered neutron stars that showed magnetar-like variability, a particularly interesting case is that of PSR B0943+10. Recent observations have shown that this pulsar, well studied in the radio band where it alternates between a bright and a quiescent mode, displays significant X-ray variations, anticorrelated in flux with the radio emission. The study of such synchronous radio/X-ray mode switching opens a new window to investigate the processes responsible for the pulsar radio and high-energy emission. Here we review the main X-ray properties of PSR B0943+10 derived from recent coordinated X-ray and radio observations." @default.
• W2754366346 created "2017-09-25" @default.
• W2754366346 creator A5014665960 @default.
• W2754366346 creator A5042567253 @default.
• W2754366346 date "2017-09-01" @default.
• W2754366346 modified "2023-10-09" @default.
• W2754366346 title "The Radio and X-ray Mode-Switching Pulsar PSR B0943+10" @default.
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• W2754366346 doi "https://doi.org/10.1007/s12036-017-9464-7" @default.
• W2754366346 hasPublicationYear "2017" @default.
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