中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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
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
DOI10.1051/0004-6361/202348821
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

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。