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DOI | 10.1093/mnras/stv2456 |
Jet-driven outflows of ionized gas in the nearby radio galaxy 3C 293 | |
Mahony, E. K.1; Oonk, J. B. R.1,2; Morganti, R.1,3; Tadhunter, C.4; Bessiere, P.5; Short, P.4; Emonts, B. H. C.6; Oosterloo, T. A.1,3 | |
通讯作者 | Mahony, E. K. |
来源期刊 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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ISSN | 0035-8711 |
EISSN | 1365-2966 |
出版年 | 2016 |
卷号 | 455期号:3页码:2453-2460 |
英文摘要 | Fast outflows of gas, driven by the interaction between the radio jets and interstellar medium (ISM) of the host galaxy, are being observed in an increasing number of galaxies. One such example is the nearby radio galaxy 3C 293. In this paper we present integral field unit observations taken with OASIS on the William Herschel Telescope, enabling us to map the spatial extent of the ionized gas outflows across the central regions of the galaxy. The jet-driven outflow in 3C 293 is detected along the inner radio lobes with a mass outflow rate ranging from similar to 0.05 to 0.17 M-circle dot yr(-1) (in ionized gas) and corresponding kinetic power of similar to 0.5-3.5 x 10(40) erg s(-1). Investigating the kinematics of the gas surrounding the radio jets (i.e. not directly associated with the outflow), we find linewidths broader than 300 km s(-1) up to 5 kpc in the radial direction from the nucleus (corresponding to 3.5 kpc in the direction perpendicular to the radio axis at maximum extent). Along the axis of the radio jet linewidths >400 km s(-1) are detected out to 7 kpc from the nucleus and linewidths of >500 km s(-1) at a distance of 12 kpc from the nucleus, indicating that the disturbed kinematics clearly extend well beyond the high surface brightness radio structures of the jets. This is suggestive of the cocoon structure seen in simulations of jet-ISM interaction and implies that the radio jets are capable of disturbing the gas throughout the central regions of the host galaxy in all directions. |
英文关键词 | ISM: jets and outflows galaxies: individual: 3C 293 galaxies: ISM galaxies: jets radio lines: galaxies radio lines: ISM |
类型 | Article |
语种 | 英语 |
国家 | Netherlands ; England ; Chile ; Spain |
收录类别 | SCI-E |
WOS记录号 | WOS:000368008200015 |
WOS关键词 | ACTIVE GALACTIC NUCLEI ; MOLECULAR GAS ; STAR-FORMATION ; BLACK-HOLES ; COLD GAS ; NGC 1266 ; NEUTRAL HYDROGEN ; WARM OUTFLOW ; FEEDBACK ; 3C-293 |
WOS类目 | Astronomy & Astrophysics |
WOS研究方向 | Astronomy & Astrophysics |
资源类型 | 期刊论文 |
条目标识符 | http://119.78.100.177/qdio/handle/2XILL650/195125 |
作者单位 | 1.Netherlands Inst Radio Astron, ASTRON, NL-7990 AA Dwingeloo, Netherlands; 2.Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands; 3.Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands; 4.Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England; 5.Univ Concepcion, Dept Astron, Concepcion, Chile; 6.Ctr Astrobiol INTA CSIC, E-28850 Madrid, Spain |
推荐引用方式 GB/T 7714 | Mahony, E. K.,Oonk, J. B. R.,Morganti, R.,et al. Jet-driven outflows of ionized gas in the nearby radio galaxy 3C 293[J],2016,455(3):2453-2460. |
APA | Mahony, E. K..,Oonk, J. B. R..,Morganti, R..,Tadhunter, C..,Bessiere, P..,...&Oosterloo, T. A..(2016).Jet-driven outflows of ionized gas in the nearby radio galaxy 3C 293.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,455(3),2453-2460. |
MLA | Mahony, E. K.,et al."Jet-driven outflows of ionized gas in the nearby radio galaxy 3C 293".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 455.3(2016):2453-2460. |
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