The geometry of intermittent and magnetospheric state changes pulsars
Context. Pulsars exhibit a variety of phenomena, including intermittency and magnetospheric state changes (MSC) – moding, nulling, and profile $ {\dot {\nu }} $-correlation – which are thought to be related to changes in their magnetospheric plasma.
Weltevrede, P. +14 more
core +1 more source
Spin effects in superfluidity, neutron matter, and neutron stars. [PDF]
Sedrakian A, Rau PB.
europepmc +1 more source
Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262. [PDF]
Kong L +14 more
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AI-powered drone-based automated inspection of FAST. [PDF]
Wang L.
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Stochastic analysis of compact stars under composite polytropes. [PDF]
Nouh MI +3 more
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Cross-Feature Hybrid Associative Priori Network for Pulsar Candidate Screening. [PDF]
Luo W, Xie X, Jiang J, Zhou L, Hu Z.
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Reading signatures of supermassive binary black holes in pulsar timing array observations. [PDF]
Goncharov B +12 more
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Estimation of mass and radii for charged compact objects using a modified Chaplygin equation of state in the Buchdahl-I metric. [PDF]
Zahra A +4 more
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Direct spectroscopic observation of matter falling onto a compact stellar object. [PDF]
Rahin R +12 more
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Adaptive Orbital Rendezvous Control of Multiple Satellites Based on Pulsar Positioning Strategy. [PDF]
Chen Q, Zhao Y, Yan L.
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