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Spin period evolution of Vela pulsar based on the wind emission: Application to the long period radio pulsars GPM J1839‐10 (P = 21 min) and GLEAM‐X J1627 (P = 18 min)
Inferring neutron star properties with continuous gravitational waves
Neil Lu, Karl Wette, Susan M Scott and Andrew Melatos Monthly Notices of the Royal Astronomical Society 521(2) 2103 (2023) https://doi.org/10.1093/mnras/stad390
Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque
Cheng-Min Zhang, Xiang-Han Cui, Di Li, De-Hua Wang, Shuang-Qiang Wang, Na Wang, Jian-Wei Zhang, Bo Peng, Wei-Wei Zhu, Yi-Yan Yang and Yuan-Yue Pan Universe 8(12) 628 (2022) https://doi.org/10.3390/universe8120628
Revisiting the Magnetic Field Distribution of Normal Pulsars: Implications for the Multiple Origins for Neutron Stars
Jianwei Zhang, Chengmin Zhang, Di Li, et al. Publications of the Astronomical Society of the Pacific 134(1041) 114201 (2022) https://doi.org/10.1088/1538-3873/ac9ad8
The illusion of neutron star magnetic field estimates
A. G. Lyne, C. A. Jordan, F. Graham-Smith, et al. Monthly Notices of the Royal Astronomical Society 446(1) 857 (2015) https://doi.org/10.1093/mnras/stu2118