The variability of radio pulsars
Neutron stars are amongst the most exotic objects known in the universe; more than a solar mass of material is squeezed into an object the size of a city, leading to a density comparable to that of an atomic nucleus. They have a surface magnetic field which is typically around a trillion times stronger than the magnetic field here on Earth, and we have
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Radio Emission across the Entire Rotation Phases of Pulsars
Supersensitive observations of bright pulsars by the Five-hundred-meter Aperture Spherical Telescope have revealed weak radio emission continuously emerges in the rotation phases between the “main” pulse and “interpulse” of a rotating neutron star.
P. F. Wang, J. L. Han
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An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers. [PDF]
Pang PTH +20 more
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A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism. [PDF]
Zhu W +36 more
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The evolution of radio pulsars [PDF]
B. N. Candy, D. G. Blair
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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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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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Performance of the Sardinia Radio Telescope Using the Dual-Polarized Cryogenic C-Low Receiver in the 4.2-5.6 GHz Frequency Band. [PDF]
Schirru L +16 more
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Stochastic analysis of compact stars under composite polytropes. [PDF]
Nouh MI +3 more
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The impact of FAST on the research of fast radio bursts. [PDF]
Xu R.
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