Spider pulsars are a subclass of millisecond pulsar binary systems with low mass companions in short-period orbits. In spider pulsars, the pulsar wind and electromagnetic emission ablate and may destroy the companion. The study of spider pulsars offers valuable opportunities to investigate the characteristics of the companion stars under intense irradiation. 

Researchers from the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences successfully measured the magnetic field of a spider pulsar PSR J2051-0827. 

The study was  published in the Astrophysical Journal on Sept. 14.

Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), the researchers investigated the polarization properties of a spider pulsar PSR J2051-0827 and found direct evidence of the existence of magnetic field in the eclipse medium of PSR J2051-0827. 

During the egress of the eclipse of PSR J2051-0827, the researchers found that there is a regular decrease in rotation measure (RM), which changes from 60 to -28.7 rad m-2This regular decrease in RM suggests that there is a significant magnetic field in the eclipse medium. The line-of-sight magnetic field strength is estimated to be 0.1 G based on the variation of RM. Considering the magnetic field levels in the eclipse medium, they concluded that cyclotron damping may not be the primary eclipse mechanism at the L-band.

Furthermore,the RM reversal phenomenon is also detected, which could be caused by a change in the magnetic field strength along the line of sight due to binary orbital motion. The RM reversal phenomenon provides evidence for a complicated, magnetized immediate environment of the source. The results suggest that environments of spider pulsars share some similarities with some fast radio bursts (FRBs). 

The polarization properties of PSR J2051-0827 vs. orbital

Contact: WANG Shuangqiang

Xinjiang Astronomical Observatory, Chinese Academy of Sciences

E-mail：wangshuangqiang@xao.ac.cn

Article link: https://doi.org/10.3847/1538-4357/acea81