Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: dynamics [PDF]
, 2019 Barbara Olmi, N. Bucciantini
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The optical counterparts of accreting millisecond X-ray pulsars during quiescence [PDF]
, 2009 P. D'Avanzo +5 more
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The Dawes Review 11: From young to old: The evolutionary path of Pulsar Wind Nebulae – CORRIGENDUM [PDF]
, 2023 Barbara Olmi, N. Bucciantini
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HST/STIS analysis of the first main sequence pulsar CU Virginis [PDF]
, 2019 J. Krtička +11 more
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Observations of the Pulsar Wind Nebula HESS J1825–137 with H.E.S.S. II [PDF]
, 2017 Alison Mitchell +5 more
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White Dwarf Pulsars as Possible Gamma-Ray Sources [PDF]
, 2019 P. J. Meintjes +4 more
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A Lower Mass Estimate for PSR J0348+0432 Based on CHIME/Pulsar Precision Timing
The Astrophysical Journal LettersThe binary pulsar J0348+0432 was previously shown to have a mass of approximately 2 M _⊙ , based on the combination of radial-velocity and model-dependent mass parameters derived from high-resolution optical spectroscopy of its white-dwarf companion.
Alexander Saffer +10 more
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Applied SciencesPulsars are neutron stars with high rotation speeds and have extraordinary long-term rotational stability. X-ray pulsar-based navigation (XNAV) is a navigation method that estimates the position and velocity of a spacecraft using the X-ray radiation from
Kun Jiang +3 more
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Burst-recurrence properties revealed with Insight-HXMT and NICER for the newly discovered accreting millisecond pulsar MAXI J1816–195 [PDF]
Peng-Ju Wang +14 more
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An Explanation of Anomalous Velocities in Pulsar Scintillation Patterns [PDF]
, 1975 B. J. Uscinski
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