Arid
DOI10.1093/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
ISSN0035-8711
EISSN1365-2966
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
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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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