On the Nature of Long Period Radio Pulsar GPM J1839-10:Death Line and Pulse Width

作     者：H.Tong H.Tong

作者机构：School of Physics and Materials ScienceGuangzhou UniversityGuangzhou 510006China 

出 版 物：《Research in Astronomy and Astrophysics》 (天文和天体物理学研究（英文版）)

年 卷 期：2023年第23卷第12期

页      面：215-220页

核心收录：

学科分类：07[理学] 070401[理学-天体物理] 0704[理学-天文学] 

基　　金：supported by National SKA Program of China(No.2020SKA0120300) the National Natural Science Foundation of China(NSFC,12133004) 

主　　题：stars magnetars-(stars:)pulsars general-(stars:)pulsars individual(GPM J1839−10) 

摘      要：Recently another long period radio pulsar GPM J1839-10 has been reported,similar to GLEAM-X ***,the energy budget and rotational evolution of long period radio pulsars had been *** time,the death line and pulse width for neutron star and white dwarf pulsars are *** pulse width is included as the second criterion for neutron star and white dwarf *** is found that:(1)PSR J0250+5854 and PSR J0901-4046 *** be normal radio *** have narrow pulse width and they lie near the radio emission death line.(2)The two long period radio pulsars GLEAM-X J162759.5-523504.3 and GPM J1839-10 are unlikely to be normal radio *** possible pulse width is relatively *** lie far below the fiducial death line on the P-P^(·)diagram.(3)GLEAM-X J162759.5-523504.3 and GPM J1839-10 may be magnetars or white dwarf radio *** present,there are many parameters and uncertainties in both of these possibilities.