A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030
文献类型:期刊论文
作者 | Gorski, M. D.2,22,23; Aalto, S.22; Konig, S.22; Wethers, C. F.22; Yang, C.22; Muller, S.22; Onishi, K.1,22; Sato, M.22; Falstad, N.22; Mangum, J. G.21 |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2024-04-10 |
卷号 | 684页码:L11 |
关键词 | galaxies: evolution galaxies: ISM galaxies: clusters: individual: ESO 320-G030 galaxies: nuclei galaxies: structure |
ISSN号 | 0004-6361 |
DOI | 10.1051/0004-6361/202348821 |
产权排序 | 14 |
英文摘要 | How galaxies regulate nuclear growth through gas accretion by supermassive black holes (SMBHs) is one of the most fundamental questions in galaxy evolution. One potential way to regulate nuclear growth is through a galactic wind that removes gas from the nucleus. It is unclear whether galactic winds are powered by jets, mechanical winds, radiation, or via magnetohydrodynamic (MHD) processes. Compact obscured nuclei represent a significant phase of galactic nuclear growth. These galaxies hide growing SMBHs or unusual starbursts in their very opaque, extremely compact (r < 100 pc) centres. They are found in approximately 30% of the luminous and ultra-luminous infrared galaxy population. Here, we present high-resolution ALMA observations (similar to 30 mas, similar to 5 pc) of ground-state and vibrationally excited HCN towards ESO 320-G030 (IRAS 11506-3851). ESO 320-G030 is an isolated luminous infrared galaxy known to host a compact obscured nucleus and a kiloparsec-scale molecular wind. Our analysis of these high-resolution observations excludes the possibility of a starburst-driven wind, a mechanically or energy driven active galactic nucleus wind, and exposes a molecular MDH wind. These results imply that the nuclear evolution of galaxies and the growth of SMBHs are similar to the growth of hot cores or protostars where gravitational collapse of the nuclear torus drives a MHD wind. These results mean galaxies are capable, in part, of regulating the evolution of their nuclei without feedback. |
WOS关键词 | EXTENDED MOLECULAR OUTFLOW ; AGN-DRIVEN OUTFLOW ; STAR-FORMATION ; RESOLUTION OBSERVATIONS ; INFRARED GALAXIES ; ALMA IMAGES ; BLACK-HOLES ; X-RAY ; NUCLEI ; EMISSION |
资助项目 | Swedish Research Council[621-2011-4143] ; Swedish Research Council[2017-00648] ; European Research Council (ERC) under the European Union[789410] ; European Research Council (ERC) under the European Union[833460] ; Nordic ALMA Regional Center (ARC) ; Spanish Ministerio de Economa y Competitividad[PID2019-105552RB-C41] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001199982500013 |
出版者 | EDP SCIENCES S A |
资助机构 | Swedish Research Council ; European Research Council (ERC) under the European Union ; Nordic ALMA Regional Center (ARC) ; Spanish Ministerio de Economa y Competitividad |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/6763] ![]() |
专题 | 恒星形成与演化研究团组 |
通讯作者 | Gorski, M. D. |
作者单位 | 1.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 2.Northwestern Univ, CIERA, Evanston, IL 60208 USA 3.Univ Alcala, Dept Fis & Matemat, Campus Univ, Madrid 28871, Spain 4.Univ Wisconsin, Dept Astron, 475 North Charter St, Madison, WI 53706 USA 5.European Univ Cyprus, Sch Sci, Diogenes St, CY-1516 Nicosia, Cyprus 6.Fdn Res & Technol Hellas FORTH, Inst Astrophys, Iraklion 70013, Greece 7.SOKENDAI, Astron Sci Program, Grad Inst Adv Studies, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 8.UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England 9.King Abdulaziz Univ, Fac Sci, Astron Dept, POB 80203, Jeddah 21589, Saudi Arabia 10.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China |
推荐引用方式 GB/T 7714 | Gorski, M. D.,Aalto, S.,Konig, S.,et al. A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030[J]. ASTRONOMY & ASTROPHYSICS,2024,684:L11. |
APA | Gorski, M. D..,Aalto, S..,Konig, S..,Wethers, C. F..,Yang, C..,...&Gonzalez-Alfonso, E..(2024).A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030.ASTRONOMY & ASTROPHYSICS,684,L11. |
MLA | Gorski, M. D.,et al."A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030".ASTRONOMY & ASTROPHYSICS 684(2024):L11. |
入库方式: OAI收割
来源:新疆天文台
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