NAOC Open IR
Constraints on the kinetic energy of type-Ic supernova explosion from young PSR J1906+0746 in a double neutron star candidate*
Yang, Yi-Yan1; Zhang, Cheng-Min2; Zhang, Jian-Wei3; Wang, De-Hua4
2021-06-01
Source PublicationCHINESE PHYSICS B
ISSN1674-1056
Volume30Issue:6Pages:6
AbstractSo far among the nineteen pairs of detected double neutron star (DNS) systems, it is a usual fact that the first-born recycled pulsar is detected, however the youngest DNS system PSR J1906+0746, with the characteristic age of 113 kyr, is one of the three detected DNS as a non-recycled and second-born NS, which is believed to be formed by an electron capture or a low energy ultra-stripped iron core-collapse supernova (SN) explosion. The SN remnant around PSR J1906+0746 is too dim to be observed by optical telescopes, then its x-ray flux limit has been given by Chandra. A reference pulsar PSR J1509-5850 with the young characteristic age of 154 kyr was chosen as an object of comparison, which has an SN remnant observed by Chandra and is believed to be formed by iron core SN explosion. We impose a restriction on the maximum kinetic energy of electron-capture (EC) SN explosion that induces the formation of PSR J1906+0746. The estimated result is (4-8)x10(50) erg (1 erg = 10(-7) J), which is consistent with that of the published simulations of the EC process, i.e., a lower value than that of the conventional iron core SN explosion of (1-2) x 10(51) erg. As suggested, EC process for NS formation is pertained to the subluminous type Ic SN by the helium star with ONeMg core, thus for the first time we derived the kinetic energy of EC SN explosion of DNS, which may be reconciled with the recent observation of type Ic SN 2014ft with kinetic energy of 2 x 10(50) erg.
Keywordneutron star pulsar astrophysics high energy astrophysical phenomena
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; Project of Guizhou Provincial Education Department ; Project of Guizhou Provincial Education Department ; Doctoral Project of Guizhou Education University ; Doctoral Project of Guizhou Education University ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; Project of Guizhou Provincial Education Department ; Project of Guizhou Provincial Education Department ; Doctoral Project of Guizhou Education University ; Doctoral Project of Guizhou Education University ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; Project of Guizhou Provincial Education Department ; Project of Guizhou Provincial Education Department ; Doctoral Project of Guizhou Education University ; Doctoral Project of Guizhou Education University ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; Project of Guizhou Provincial Education Department ; Project of Guizhou Provincial Education Department ; Doctoral Project of Guizhou Education University ; Doctoral Project of Guizhou Education University ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China
DOI10.1088/1674-1056/abda2c
WOS KeywordELECTRON-CAPTURE SUPERNOVAE ; MERGER RATE ; PULSAR ; EVOLUTION ; BINARY ; KICKS
Language英语
Funding ProjectNational Natural Science Foundation of China[U1938117] ; National Natural Science Foundation of China[U1731238] ; National Natural Science Foundation of China[11703003] ; National Natural Science Foundation of China[11647114] ; International Partnership Program of Chinese Academy of Sciences[114A11KYSB20160008] ; National Key Research and Development Program of China[2016YFA0400702] ; Guizhou Provincial Science and Technology Foundation[[2020]1Y019] ; Project of Guizhou Provincial Education Department[[2018]058] ; Doctoral Project of Guizhou Education University[2020BS021] ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China[ZDXK[2015]38]
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; Project of Guizhou Provincial Education Department ; Project of Guizhou Provincial Education Department ; Doctoral Project of Guizhou Education University ; Doctoral Project of Guizhou Education University ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; Project of Guizhou Provincial Education Department ; Project of Guizhou Provincial Education Department ; Doctoral Project of Guizhou Education University ; Doctoral Project of Guizhou Education University ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; Project of Guizhou Provincial Education Department ; Project of Guizhou Provincial Education Department ; Doctoral Project of Guizhou Education University ; Doctoral Project of Guizhou Education University ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Guizhou Provincial Science and Technology Foundation ; Guizhou Provincial Science and Technology Foundation ; Project of Guizhou Provincial Education Department ; Project of Guizhou Provincial Education Department ; Doctoral Project of Guizhou Education University ; Doctoral Project of Guizhou Education University ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China ; Key Support Disciplines of Theoretical Physics of Department of Education of Guizhou Province, China
WOS Research AreaPhysics
WOS SubjectPhysics, Multidisciplinary
WOS IDWOS:000662678600001
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/77473
Collection中国科学院国家天文台
Corresponding AuthorYang, Yi-Yan; Zhang, Cheng-Min
Affiliation1.Guizhou Educ Univ, Sch Phys & Elect Sci, Guiyang 550018, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, CAS Key Lab FAST, Beijing 100012, Peoples R China
3.Beijing Normal Univ, Astron Dept, Beijing 100875, Peoples R China
4.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China
Recommended Citation
GB/T 7714
Yang, Yi-Yan,Zhang, Cheng-Min,Zhang, Jian-Wei,et al. Constraints on the kinetic energy of type-Ic supernova explosion from young PSR J1906+0746 in a double neutron star candidate*[J]. CHINESE PHYSICS B,2021,30(6):6.
APA Yang, Yi-Yan,Zhang, Cheng-Min,Zhang, Jian-Wei,&Wang, De-Hua.(2021).Constraints on the kinetic energy of type-Ic supernova explosion from young PSR J1906+0746 in a double neutron star candidate*.CHINESE PHYSICS B,30(6),6.
MLA Yang, Yi-Yan,et al."Constraints on the kinetic energy of type-Ic supernova explosion from young PSR J1906+0746 in a double neutron star candidate*".CHINESE PHYSICS B 30.6(2021):6.
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