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A magnetohydrodynamical model for the formation of episodic jets
Yuan, F1; Lin J(林隽)2,3; Wu, KW4; Ho, LC5; Yuan, F (reprint author), Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, JOINGC SHAO & USTC, 80 Nandan Rd, Shanghai 200030, Peoples R China.
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2009-06-01
卷号395期号:4页码:2183-2188
DOI10.1111/j.1365-2966.2009.14673.x
产权排序第2完成单位
收录类别SCI
关键词Black Hole Physics Accretion Mhd Accretion Discs Ism: Jets And Outflow
摘要Episodic ejection of plasma blobs has been observed in many black hole systems. While steady, continuous jets are believed to be associated with large-scale open magnetic fields, what causes the episodic ejection of blobs remains unclear. Here by analogy with the coronal mass ejection on the Sun, we propose a magnetohydrodynamical model for episodic ejections from black holes associated with the closed magnetic fields in an accretion flow. Shear and turbulence of the accretion flow deform the field and result in the formation of a flux rope in the disc corona. Energy and helicity are accumulated and stored until a threshold is reached. The system then loses its equilibrium and the flux rope is thrust outward by the magnetic compression force in a catastrophic way. Our calculations show that for parameters appropriate for the black hole in our Galactic centre, the plasmoid can attain relativistic speeds in about 35 min.
项目资助者Natural Science Foundation of China [10773024, 10833002, 10821302, 10825314, 10873030, 40636031] ; One-Hundred-Talent Program of CAS ; National Basic Research Program of China [2009CB824800, 2006CB806303] ; Chinese Academy of Sciences [KJCX2-YWT04] ; NASA [NNX07AL72G]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0035-8711
URL查看原文
WOS记录号WOS:000266112600034
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]MAGNETICALLY DRIVEN ACCRETION ; ADVECTION-DOMINATED ACCRETION ; CORONAL MASS EJECTIONS ; BLACK-HOLES ; SAGITTARIUS-A ; SOLAR ERUPTIONS ; GRS 1915+105 ; DISKS ; FLOWS ; FIELD
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被引频次:63[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/6136
专题太阳物理研究组
通讯作者Yuan, F (reprint author), Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, JOINGC SHAO & USTC, 80 Nandan Rd, Shanghai 200030, Peoples R China.
作者单位1.Joint Institute for Galaxy and Cosmology (JOINGC) of SHAO and USTC, Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
2.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China
3.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
4.Mullard Space Science Laboratory, University College London, Holmbury St Mary, Surrey RH5 6NT
5.The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101, USA
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Yuan, F,Lin J,Wu, KW,et al. A magnetohydrodynamical model for the formation of episodic jets[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2009,395(4):2183-2188.
APA Yuan, F,Lin J,Wu, KW,Ho, LC,&Yuan, F .(2009).A magnetohydrodynamical model for the formation of episodic jets.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,395(4),2183-2188.
MLA Yuan, F,et al."A magnetohydrodynamical model for the formation of episodic jets".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 395.4(2009):2183-2188.
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