FAST Telescope Reveals Emission Properties of Three Long-Period Pulsars in New Study
The emission properties of three long-period pulsars have been observed through the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Detailed findings of the study highlight various pulsar emission behaviours, including null phases, asymmetric emissions, and microstructure pulses. The research, conducted as part of the Commensal Radio Astronomy FAST Survey (CRAFTS), aimed to deepen the understanding of pulsar magnetospheric activity and emission mechanisms. The pulsars under examination—PSR J1945+1211, PSR J2323+1214, and PSR J1900−0134—were observed across a frequency range of 1.05 to 1.45 GHz using FAST’s 19-beam receiver. These observations provided crucial insights into the nature of their radio pulses and periodicity. Observations of Pulsar Null Phases According to the study published on the arXiv preprint server, quasi-periodic nulling phenomena were detected in all three pulsars, with durations varying from 57 to 71.44 seconds. The null fractions for PSR J1945+1211, PSR J2323+1214, and PSR J1900−0134 were determined to be 52.46 percent, 48.48 percent, and 27.51 percent, respectively. Nulling, which refers to temporary reductions or cessations in emission, is a key characteristic observed in pulsars and is essential for …

