Institutional Repository of Radio Astronomy Research Laboratory
| Explaining the 'Outliers' Track in Black Hole X-ray Binaries with a BZ-Jet and Inner-Disk Coupling | |
Chang, Ning1,2 ; Liu, Xiang1,3,4; Xie, Fu-Guo5; Cui, Lang1,3,4; Shan, Hao1
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| 2022-06-01 | |
| Source Publication | UNIVERSE
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| Volume | 8Issue:6Pages:333 |
| Contribution Rank | 1 |
| Abstract | In this paper, we investigate the black hole (BH) spin contribution to jet power, especially for the magnetic arrested disk (MAD), where only inner accretion disk luminosity is closely coupled with the spin-jet power, and try to explain the 'outliers' track of the radio L-R to X-ray luminosity L-X in two black hole X-ray binaries (BHXBs). Our results suggest that the BZ-jet and the inner-disk coupling could account for the 'outliers' track of the radio/X-ray correlation in two BHXBs, H1743-322 and MAXI J1348-630. Although the accretion disk of H1743-322 in the outburst could be in the MAD state, there is a lower probability that MAXI J1348-630 is in the MAD state due to its low jet production efficiency. The difference in the inner-disk bolometric luminosity ratio of the two sources implies that these two BHXBs are in different inner-disk accretion states. We further investigate the phase-changing regime of MAXI J1348-630 and find that there is a phase transition around L-X/L-Edd similar to 10(-3). The assumption of sub-MAD is discussed as well. |
| Keyword | accretion disk black hole physics X-ray binaries radio jets |
| DOI | 10.3390/universe8060333 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | RADIATIVELY INEFFICIENT ACCRETION ; ACTIVE GALACTIC NUCLEI ; MAGNETOHYDRODYNAMIC SIMULATIONS ; COLLAPSING STAR ; HARD-STATE ; RADIO ; LUMINOSITY ; OUTBURST ; MATTER ; FLOWS |
| Funding Project | National Key R&D Program of China[2018YFA0404602] ; National SKA Program of China[2020SKA0110102] ; Youth Innovation Promotion Association of CAS[Y202064] ; Chinese Academy of Sciences (CAS) 'Light ofWest China' Program[2021-XBQNXZ-005] ; National Natural Science Foundation of China[11673056] ; National Natural Science Foundation of China[11173042] |
| WOS Research Area | Astronomy & Astrophysics ; Physics |
| WOS Subject | Astronomy & Astrophysics ; Physics, Particles & Fields |
| WOS ID | WOS:000817635800001 |
| Publisher | MDPI |
| Funding Organization | National Key R&D Program of China ; National SKA Program of China ; Youth Innovation Promotion Association of CAS ; Chinese Academy of Sciences (CAS) 'Light ofWest China' Program ; National Natural Science Foundation of China |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/4827 |
| Collection | 射电天文研究室_星系宇宙学研究团组 |
| Corresponding Author | Liu, Xiang |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China 2.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China 3.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China 4.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China 5.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Chang, Ning,Liu, Xiang,Xie, Fu-Guo,et al. Explaining the 'Outliers' Track in Black Hole X-ray Binaries with a BZ-Jet and Inner-Disk Coupling[J]. UNIVERSE,2022,8(6):333. |
| APA | Chang, Ning,Liu, Xiang,Xie, Fu-Guo,Cui, Lang,&Shan, Hao.(2022).Explaining the 'Outliers' Track in Black Hole X-ray Binaries with a BZ-Jet and Inner-Disk Coupling.UNIVERSE,8(6),333. |
| MLA | Chang, Ning,et al."Explaining the 'Outliers' Track in Black Hole X-ray Binaries with a BZ-Jet and Inner-Disk Coupling".UNIVERSE 8.6(2022):333. |
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| Chang-2022-Explainin（602KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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