KMS National Astronomical Observatories, CAS
Estimating the masses of three neutron stars by twin kilohertz quasi-periodic oscillations and innermost stable circular orbits: constraining equations of state | |
Shi, Chang-Sheng1; Zhang, Shuang-Nan2,3,4 | |
2020-05-01 | |
Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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ISSN | 0035-8711 |
Volume | 494Issue:3Pages:4382-4392 |
Abstract | We test the magnetohydrodynamics (MHD) model derived by Shi, Zhang and Li by the like-standard deviations of the twin kilohertz (kHz) quasi-periodic oscillation (QPO) frequencies when the modes of the MHD waves in the MHD model are recalculated. A group of approximate equations derived from the MILD equations in the MILD model are proposed. Consequently, the dependence of the twin kHz QPO frequencies on several neutron star (NS) parameters is determined by the approximate equations. Based on the selection criterion that NS parameters corresponding to the minimum like-standard deviation are the most reasonable parameters, the masses of the three NSs in 4U 0614+09, 4U 1636-53 and 4U 1608-52 are estimated as M < 2.60 M-circle dot, 2.00 M-circle dot < M < 2.31 M-circle dot and 2.17 M-circle dot < M < 2.62 M-circle dot, respectively. According to these NS masses, some equations of state for the nuclear matter in compact stars can be ruled out. |
Keyword | accretion, accretion discs MHD X-rays: binaries stars: neutron stars: magnetic field equation of state |
Funding Organization | National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; program of China Scholarships Council ; program of China Scholarships Council ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; program of China Scholarships Council ; program of China Scholarships Council ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; program of China Scholarships Council ; program of China Scholarships Council ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; program of China Scholarships Council ; program of China Scholarships Council ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS |
DOI | 10.1093/mnras/staa802 |
WOS Keyword | ATOLL SOURCE STATES ; X-RAY BINARIES ; BLACK-HOLES ; 4U 1636-53 ; OF-STATE ; FREQUENCY ; MODEL ; ACCRETION ; PULSARS ; RADII |
Language | 英语 |
Funding Project | National Program on Key Research and Development Project[2016YFA0400802] ; National Natural Science Foundation of China[11563003] ; National Natural Science Foundation of China[U1838202] ; program of China Scholarships Council[201907565014] ; Key Research Program of Frontier Sciences, CAS[QYZDY-SSW-SLH008] |
Funding Organization | National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; program of China Scholarships Council ; program of China Scholarships Council ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; program of China Scholarships Council ; program of China Scholarships Council ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; program of China Scholarships Council ; program of China Scholarships Council ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; program of China Scholarships Council ; program of China Scholarships Council ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000535882100099 |
Publisher | OXFORD UNIV PRESS |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.bao.ac.cn/handle/114a11/54746 |
Collection | 中国科学院国家天文台 |
Corresponding Author | Shi, Chang-Sheng |
Affiliation | 1.Hainan Univ, Sch Sci, Haikou 570228, Hainan, Peoples R China 2.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China |
Recommended Citation GB/T 7714 | Shi, Chang-Sheng,Zhang, Shuang-Nan. Estimating the masses of three neutron stars by twin kilohertz quasi-periodic oscillations and innermost stable circular orbits: constraining equations of state[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,494(3):4382-4392. |
APA | Shi, Chang-Sheng,&Zhang, Shuang-Nan.(2020).Estimating the masses of three neutron stars by twin kilohertz quasi-periodic oscillations and innermost stable circular orbits: constraining equations of state.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,494(3),4382-4392. |
MLA | Shi, Chang-Sheng,et al."Estimating the masses of three neutron stars by twin kilohertz quasi-periodic oscillations and innermost stable circular orbits: constraining equations of state".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 494.3(2020):4382-4392. |
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