中文
相关论文

相关论文: Gas outflows in radio galaxies

200 篇论文

AGN activity is known to drive fast outflows of gas. We report the discovery of fast outflows of neutral gas with velocities over 1000 km/s in a number of radio galaxies. In the best studied object, 3C~293, the kinematical properties of the…

天体物理学 · 物理学 2009-11-10 T. A. Oosterloo , R. Morganti , B. H. C. Emonts , C. N. Tadhunter

Outflows up to 1500 km/s of atomic neutral hydrogen are detected in a growing number of radio galaxies. Outflows with similar velocities are also detected in ionized gas, suggesting a common origin for the extreme kinematics of these two…

天体物理学 · 物理学 2007-05-23 R. Morganti , T. Oosterloo , C. Tadhunter

Fast (~1000 km/s) outflows of neutral gas (from 21-cm HI absorption) are detected in strong radio sources. The outflows occur, at least in some cases, at distances from the radio core that range between few hundred parsecs and kpc. These HI…

天体物理学 · 物理学 2007-05-23 Raffaella Morganti , Clive Tadhunter , Tom Oosterloo , Joanna Holt , Bjorn Emonts

We report the detection of fast (~ 1000 km/s), massive outflows of neutral gas observed -- using the WSRT -- as 21-cm HI absorption against the strong radio continuum of seven radio sources. The neutral outflows occur, in at least somes…

天体物理学 · 物理学 2009-11-11 R. Morganti , C. N. Tadhunter , T. A. Oosterloo

AGN feedback is now a major component of models of galaxy evolution. Using near-infrared imaging spectroscopy on the VLT we identify kpc-sized outflows of few x 10^10 M_s of ionized gas in powerful radio galaxies at z~2-3. Velocity fields…

宇宙学与河外天体物理 · 物理学 2009-06-19 N. P. H. Nesvadba

The study of the conditions and the kinematics of the gas in the central region of AGN provides important information on the relevance of feedback effects connected to the nuclear activity. Quantifying these effects is key for constraining…

宇宙学与河外天体物理 · 物理学 2015-05-18 Raffaella Morganti , Joanna Holt , Clive Tadhunter , Tom Oosterloo

An increasing number of observations and simulations suggests that low-power (<10$^{44}$ erg s$^{-1}$) jets may be a significant channel of feedback produced by active galactic nuclei (AGN), but little is known about their actual effect on…

To accommodate the seemingly "anti-hierarchical" properties of galaxies near the upper end of the mass function within our hierarchical paradigm, current models of galaxy evolution postulate a phase of vigorous AGN feedback at high…

天体物理学 · 物理学 2008-10-16 Nicole P. H. Nesvadba , Matt D. Lehnert

We explore the relationship between the ionized gas outflows and radio activity using a sample of $\sim$ 6000 AGNs at z < 0.4 with the kinematical measurement based on the [O III] line profile and the radio detection in the VLA FIRST…

星系天体物理 · 物理学 2023-06-23 Ashraf Ayubinia , Jong-Hak Woo , Suvendu Rakshit , Donghoon Son

We present four radio-loud NLS1 galaxies with extreme emission-line shifts, indicating radial outflow velocities of the ionized gas of up to 2450 km/s, above the escape velocity of the host galaxies. The forbidden lines show strong…

星系天体物理 · 物理学 2018-07-30 S. Komossa , D. W. Xu , A. Y. Wagner

Feedback from AGN is known to affect the host galaxy's evolution. In radio AGN, one manifestation of feedback is seen in gas outflows. However, it is still not well understood whether the effect of feedback evolves with the radio AGN life…

星系天体物理 · 物理学 2023-06-28 Pranav Kukreti , Raffaella Morganti , Clive Tadhunter , Francesco Santoro

Active galactic nuclei (AGN) feedback operated by the expansion of radio jets can play a crucial role in driving gaseous outflows on galaxy scales. Galaxies hosting young radio AGN, whose jets are in the first phases of expansion through…

星系天体物理 · 物理学 2021-01-04 F. Santoro , C. Tadhunter , D. Baron , R. Morganti , J. Holt

We present integral field unit (IFU) observations covering the [O III]4959,5007 and H-Beta emission lines of sixteen z<0.2 type 2 active galactic nuclei (AGN). Our targets are selected from a well-constrained parent sample of 24,000 AGN so…

星系天体物理 · 物理学 2015-06-19 C. M. Harrison , D. M. Alexander , J. R. Mullaney , A. M. Swinbank

Galaxy-scale outflows are nowadays observed in many active galactic nuclei (AGNs); however, their characterisation in terms of (multi-) phase nature, amount of flowing material, effects on the host galaxy, is still unsettled. In particular,…

星系天体物理 · 物理学 2017-10-25 Michele Perna , Giorgio Lanzuisi , Marcella Brusa , Giovanni Cresci , Marco Mignoli

Feedback from active galactic nuclei (AGN) on their host galaxies, in the form of gas outflows capable of quenching star formation, is considered a major player in galaxy evolution. However, clear observational evidence of such major impact…

星系天体物理 · 物理学 2021-04-07 Giacomo Venturi , Alessandro Marconi

The driving force behind outflows, often invoked to understand the correlation between the supermassive black holes powering active galactic nuclei (AGN) and their host galaxy properties, remains uncertain. We provide new insights into the…

星系天体物理 · 物理学 2025-03-11 Payel Nandi , C. S. Stalin , D. J. Saikia

We detect a fast outflow of neutral and ionized gas with velocities up to about 1000 km/s from the central region of radio galaxy 3C 293. With optical spectroscopy we locate the bulk of the ionized gas outflow at the position of a bright…

天体物理学 · 物理学 2007-05-23 B. H. C. Emonts , R. Morganti , T. A. Oosterloo , C. N. Tadhunter , J. M. van der Hulst

We present observations of ionized gas outflows in eleven z$ =1.39-2.59$ radio-loud quasar host galaxies. Data was taken with the integral field spectrograph (IFS) OSIRIS and the adaptive optics system at the W.M. Keck Observatory targeting…

During the last decade, wide-angle powerful outflows from AGN, both on parsec and kpc scales, have been detected in many galaxies. These outflows are widely suspected to be responsible for sweeping galaxies clear of their gas. We present…

星系天体物理 · 物理学 2012-01-18 Kastytis Zubovas , Andrew King

We investigate the ionized gas kinematics relationship with X-ray, radio and accreting properties using a sample of 348 nearby ($z < 0.4$) SDSS-FIRST-X-ray detected AGNs. X-ray properties of our sample are obtained from XMM-$Newton$,…

‹ 上一页 1 2 3 10 下一页 ›