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Rotational Evolution of the Slowest Radio Pulsar, PSR J0250+5854
Kou, F. F.1,2; Tong, H.3; Xu, R. X.4,5,6; Zhou, X.2,7
2019-05-10
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume876Issue:2Pages:131
Contribution Rank2
AbstractWe apply theoretical spin-down models of magnetospheric evolution and magnetic field decay to simulate the possible evolution of PSR J0250+5854, which is the slowest-spinning radio pulsar detected to date. Considering the alignment of inclination angle in a 3D magnetosphere, it is possible that PSR J0250+5854 has a high magnetic field comparable with magnetars or/and high magnetic field pulsars, if a small inclination angle is considered. Our calculations show that similar long-period pulsars tend to have a relatively low period derivative in this case. In another case of magnetic field decay, calculations also show a possible connection between PSR J0250+5854 and high dipole-magnetic field magnetars. The evolutionary path indicates a relatively high spin-down rate for similar long-period pulsars.
Keywordpulsars: general pulsars: individual (PSR J0250+5854) stars: neutron
DOI10.3847/1538-4357/ab17da
Indexed BySCI
Language英语
WOS KeywordMAGNETIC-FIELD DECAY ; NEUTRON-STARS ; MAGNETOTHERMAL EVOLUTION ; DEATH LINE ; EMISSION ; PERIOD
Funding ProjectNational Key R&D Program of China[2018YFA0404703] ; National Key R&D Program of China[2017YFA0402602] ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; West Light Foundation of CAS[2018-XBQNXZ-B-023] ; NSFC[11773008] ; National Natural Science Foundation of China[11873040] ; National Natural Science Foundation of China[11373006] ; National Natural Science Foundation of China[U1838108] ; National Natural Science Foundation of China[11673002] ; National Natural Science Foundation of China[U1531243] ; Strategic Priority Research Program of Chinese Academy Sciences[XDB23010200] ; Special Funding for Advanced Users
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000467818700003
PublisherIOP PUBLISHING LTD
Funding OrganizationNational Key R&D Program of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; West Light Foundation of CAS ; NSFC ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy Sciences ; Special Funding for Advanced Users
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Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/2696
Collection射电天文研究室_脉冲星研究团组
Corresponding AuthorTong, H.
Affiliation1.Chinese Acad Sci, Natl Astron Observ, CAS Key Lab FAST, Beijing 100101, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
3.Guangzhou Univ, Sch Phys & Elect Engn, Guangzhou 510006, Guangdong, Peoples R China
4.Peking Univ, Sch Phys, Beijing 100871, Peoples R China
5.Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China
6.Peking Univ, Kavil Inst Astron & Astrophys, Beijing 100871, Peoples R China
7.Chinese Acad Sci, Key Lab Radio Astron, Beijing, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Kou, F. F.,Tong, H.,Xu, R. X.,et al. Rotational Evolution of the Slowest Radio Pulsar, PSR J0250+5854[J]. ASTROPHYSICAL JOURNAL,2019,876(2):131.
APA Kou, F. F.,Tong, H.,Xu, R. X.,&Zhou, X..(2019).Rotational Evolution of the Slowest Radio Pulsar, PSR J0250+5854.ASTROPHYSICAL JOURNAL,876(2),131.
MLA Kou, F. F.,et al."Rotational Evolution of the Slowest Radio Pulsar, PSR J0250+5854".ASTROPHYSICAL JOURNAL 876.2(2019):131.
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