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Investigation on the Binary Millisecond Pulsars at Radio and gamma-Ray Wavelengths: Links with the Orbital Parameters
Wang, De-Hua1; Zhang, Cheng-Min2,3,4,5; Wang, Shuang-Qiang6
2020-07-01
Source PublicationPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
ISSN0004-6280
Volume132Issue:1013Pages:6
AbstractWe analyze the properties of the binary millisecond pulsars (BMSPs), detected at radio and gamma-ray wavelengths, and further probe their correlations with the binary orbital parameters and companion masses to trace the possible evolutionary histories. We find that the BMSPs with the lowest-mass companions, (0.006-0.06)M-circle dot, have short orbital periods P-orb < 1 day and in most cases (23 out of 25) have been detected in both radio and gamma-rays. On the other hand, the BMSPs with companion massesM(c) = (0.06-0.4)MP(orb)range, from 0.1 to 200 days, and nearly half of them show radio+gamma(53 out of 103), while the remaining ones emit only radio waves. We suggest that the two groups, with low-mass and more massive companions, respectively, experienced different evolutionary histories. Concerning the sources with the more massive companions, the radio+gamma BMSPs have on average significantly shorter spin periods (< P > = 3.37 ms) than the radio-only BMSPs (< P > = 4.73ms). We propose that the latter systems are a later evolutionary phase of the former ones.
Keywordradio pulsars neutron stars binaries pulsars gamma-rays sources
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation
DOI10.1088/1538-3873/ab9077
WOS KeywordMAGNETIC-FIELD ; NEUTRON-STAR ; EVOLUTION
Language英语
Funding ProjectNational Natural Science Foundation of China[11703003] ; National Natural Science Foundation of China[U1938117] ; National Natural Science Foundation of China[U1731238] ; Guizhou Provincial Science and Technology Foundation[[2020]1Y016]
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000541753000001
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/82952
Collection中国科学院国家天文台
Corresponding AuthorWang, De-Hua
Affiliation1.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
3.Univ Chinese Acad Sci, Sch Phys Sci, Beijing 101400, Peoples R China
4.Chinese Acad Sci, CAS Key Lab FAST, Beijing 100101, Peoples R China
5.Chinese Acad Sci, Key Lab Radio Astron, Beijing 100101, Peoples R China
6.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
Recommended Citation
GB/T 7714
Wang, De-Hua,Zhang, Cheng-Min,Wang, Shuang-Qiang. Investigation on the Binary Millisecond Pulsars at Radio and gamma-Ray Wavelengths: Links with the Orbital Parameters[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2020,132(1013):6.
APA Wang, De-Hua,Zhang, Cheng-Min,&Wang, Shuang-Qiang.(2020).Investigation on the Binary Millisecond Pulsars at Radio and gamma-Ray Wavelengths: Links with the Orbital Parameters.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,132(1013),6.
MLA Wang, De-Hua,et al."Investigation on the Binary Millisecond Pulsars at Radio and gamma-Ray Wavelengths: Links with the Orbital Parameters".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 132.1013(2020):6.
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