Subpulse Drifting of PSR J1110–5637
Subpulse Drifting of PSR J1110–5637作者机构:School of Physics and Electronic ScienceGuizhou Normal UniversityGuiyang 550001China Guizhou Provincial Key Laboratory of Radio Astronomy and Data ProcessingGuizhou Normal UniversityGuiyang 550001China School of Physics Science and TechnologyXinjiang UniversityUrumqi 830011China
出 版 物:《Research in Astronomy and Astrophysics》 (天文和天体物理学研究(英文版))
年 卷 期:2022年第22卷第6期
页 面:109-117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 Guizhou Province Science and Technology Foundation(No.ZK304) the National Natural Science Foundation of China(Nos.U1731238,11565010,12103013 and U1831120) the Foundation of Guizhou Provincial Education Department(No.KY(2020)003 and KY(2021)303) The Parkes radio telescope is part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO
主 题:(stars:)pulsars general-(stars:)pulsars individual(PSR J1110-5637)-Stars
摘 要:We report a detailed study of polarization characteristics and subpulse drifting in PSR J1110-5637 with the observations of the Parkes 64 m radio telescope at 1369 *** observations revealed that the trailing component of the pulse profile has obvious subpulse drifting,while the leading component has no subpulse *** the two-dimensional fluctuation spectrum(2DFS),we detected three distinct emission modes in the trailing component(modes A,B and C).The emission in mode A is chaotic and indistinguishable,while modes B and C have obvious subpulse *** vertical modulation periods P3of modes B and C are around the mean values of 12 P and 8 P,*** subpulse drifting of PSR J1110-5637 will expand the pulsar sample with multiple subpulse drifting rates,and this will help future systematic studies on the physical origin of the subpulse drifting phenomenon.