Download: Download full-size image Fig. 3. Number of Galactic disk MSPs discovered as a function of time. Primarily due to the surveys with a new generation of highly sensitive telescopes (FAST, MeerKAT), the discovery rate in recent years has remained as high as it has ever been. Data ...
The magnetic dipole radiation plus wind (MDRW) model for a pulsar successfully explains the evolution of the braking index between 1 and 3, by which we calculate the initial spins of the pulsars with the measured braking index, and obtain their distribution between and ms. This result is ...
Through advanced numerical techniques, we model both the dynamic and secondary spectra, providing a comprehensive framework that describes all components of the latter spectra in terms of physical quantities. Additionally, we provide a thorough analytical explanation of the secondary spectrum.Kramer Tobias...