TDB
1. Gravity experiments with radio pulsars
https://ui.adsabs.harvard.edu/abs/2024LRR....27....5F/abstract
2. PhD, Porayko, Nataliya Konstantinovna_2019_Probing the Interstellar Medium and Dark Matter with Pulsars
5. PhD, 2020, Nataliya K. PoraykoProbing the Interstellar Medium and Dark Matter with Pulsars
20241008
1 .Eclipsing Binary Pulsars
20241007
1. A 2.9-hour periodic radio transient with an optical counterpart
Hurley-Walker, N. ; McSweeney, S. J. ; Bahramian, A.
https://ui.adsabs.harvard.edu/abs/2024arXiv240815757H/abstract
The radio pulsations occur at the longest period yet found, 2.9 hours, and were discovered in archival low-frequency data from the Murchison Widefield Array (MWA).
High time resolution observations from MeerKAT show that pulsations from the source display complex microstructure and high linear polarisation, suggesting a pulsar-like emission mechanism occurring due to strong, ordered magnetic fields.
“long-period radio transients” (LPTs)
2. Long-term evolutionary links between the isolated neutron star populations
A. A. Gencali and U. Ertan
https://arxiv.org/html/2409.11595v1
We have investigated the evolutionary connections of the isolated neutron star (NS) populations including radio pulsars (RPs), anomalous X-ray pulsars (AXPs), soft gamma repeaters (SGRs), dim isolated NSs (XDINs), ‘high-magnetic field’ RPs (‘HBRPs’), central compact objects (CCOs), rotating radio transients (RRATs), and long-period pulsars (LPPs) in the fallback disc model
标签：pulsars,Notes,period,isolated,202410,radio,https,Pulsars,reading From： https://www.cnblogs.com/dejiang/p/18452227