Institutional Repository of Radio Astronomy Research Laboratory
| EOS-dependent millihertz quasi-periodic oscillation in low-mass X-ray binary | |
Liu, Helei1; Gao, Yong2,3; Li, Zhaosheng4; Dohi, Akira5,6; Wang, Weiyang2,3; Lue, Guoliang1,7 ; Xu, Renxin2,3
| |
| 2023-08-21 | |
| Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| ISSN | 0035-8711 |
| Volume | 525Issue:2Pages:2054-2068 |
| Contribution Rank | 4 |
| Abstract | We studied the frequency and critical mass accretion rate of millihertz quasi-periodic oscillations (mHz QPOs) using a one-zone X-ray burst model. The surface gravity is specified by two kinds of equation of states: neutron star (NS) and strange star (SS). The base flux, Q b, is set in the range of 0-2 MeV nucleon(-1). It is found that the frequency of mHz QPO is positively correlated to the surface gravity but negatively to the base heating. The helium mass fraction has a significant influence on the oscillation frequency and luminosity. The observed 7-9 mHz QPOs can be either explained by a heavy NS/light SS with a small base flux or a heavy SS with a large base flux. As base flux increases, the critical mass accretion rate for marginally stable burning is found to be lower. Meanwhile, the impact of metallicity on the properties of mHz QPOs was investigated using one-zone model. It shows that both the frequency and critical mass accretion rate decrease as metallicity increases. An accreted NS/SS with a higher base flux and metallicity, combined with a lower surface gravity and helium mass fraction, could be responsible for the observed critical mass accretion rate (m similar or equal to 0.3m(Edd)). The accreted fuel would be in stable burning if base flux is over than similar to 2 MeV nucleon(-1). This finding suggests that the accreting NSs/SSs in low-mass X-ray binaries showing no type I X-ray bursts possibly have a strong base heating. |
| Keyword | accretion stars:neutron star X-rays: burst |
| DOI | 10.1093/mnras/stad2424 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | NEUTRON-STAR ; NUCLEAR-EQUATION ; SHELL FLASHES ; BURSTS ; DISCOVERY ; MHZ ; MODELS ; SUPERBURST ; STABILITY ; STRANGEON |
| Funding Project | We thank the referee for the constructive feedback and comments that greatly improved the quality of this paper. We thank M. Hashimoto for his encouragement. This work received the generous support of the Major Science and Technology Program of Xinjiang Uy[12263006] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[U20312004] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[12273030] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[12288102] ; National Natural Science Foundation of China ; [2022A03013-3] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001054211400005 |
| Publisher | OXFORD UNIV PRESS |
| Funding Organization | We thank the referee for the constructive feedback and comments that greatly improved the quality of this paper. We thank M. Hashimoto for his encouragement. This work received the generous support of the Major Science and Technology Program of Xinjiang Uy ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; National Natural Science Foundation of China |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5428 |
| Collection | 射电天文研究室_理论天体物理研究团组 |
| Corresponding Author | Liu, Helei; Xu, Renxin |
| Affiliation | 1.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Peoples R China 2.Peking Univ, Dept Astron, Beijing 100871, Peoples R China 3.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 4.Xiangtan Univ, Key Lab Stars & Interstellar Medium, Xiangtan 411105, Hunan, Peoples R China 5.RIKEN, Cluster Pioneering Res, Astrophys Big Bang Lab ABBL, 2-1 Hirosawa, Wako, Saitama 3510198, Japan 6.RIKEN, Interdisciplinary Theoret & Math Sci Program iTHEM, Wako, Saitama 3510198, Japan 7.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China |
| Recommended Citation GB/T 7714 | Liu, Helei,Gao, Yong,Li, Zhaosheng,et al. EOS-dependent millihertz quasi-periodic oscillation in low-mass X-ray binary[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,525(2):2054-2068. |
| APA | Liu, Helei.,Gao, Yong.,Li, Zhaosheng.,Dohi, Akira.,Wang, Weiyang.,...&Xu, Renxin.(2023).EOS-dependent millihertz quasi-periodic oscillation in low-mass X-ray binary.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,525(2),2054-2068. |
| MLA | Liu, Helei,et al."EOS-dependent millihertz quasi-periodic oscillation in low-mass X-ray binary".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 525.2(2023):2054-2068. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Liu-2023-EOS-depende（2121KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment