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相关论文: Fast outflows in compact radio sources: evidence f…

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We report some key results from the optical emission line study of a complete sample of compact radio sources. We find strong evidence for jet-driven outflows in the circum-nuclear emission line gas namely: 1) highly broadened and…

天体物理学 · 物理学 2008-11-26 J. Holt , C. N. Tadhunter , R. Morganti

We conducted a HI 21cm absorption study of a sample of 147 nearby (z < 0.1) low-power radio sources with $10\,\mathrm{mJy} < S_{1.4\,\mathrm{GHz}} < 30\,\mathrm{mJy}$ and $\log(P_{1.4\,\mathrm{GHz}}/\mathrm{W\,Hz^{-1}}) = 20.5-23.7$, using…

星系天体物理 · 物理学 2026-03-06 Yang Su , Qingzheng Yu , Taotao Fang , Junfeng Wang , Jianfeng Wu , Bo Zhang

Using a sample of 2922 z<0.2, spectroscopically-identified Active Galactic Nuclei (AGN) we explore the relationship between radio size and the prevalence of extreme ionised outflows, as traced using broad [O III] emission-line profiles in…

星系天体物理 · 物理学 2019-11-06 S. J. Molyneux , C. M. Harrison , M. E. Jarvis

This paper reviews the evidence for interaction between radio jets and their environment in small and intermediate (sub-kpc) scale radio sources. Observations of gas (both neutral hydrogen and ionised gas) have shown the presence of fast (>…

天体物理学 · 物理学 2007-10-08 Raffaella Morganti

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

This paper is the second in a series in which we present intermediate-resolution spectra for a complete sample of 14 compact radio sources, taken with the aim of investigating the impact of the nuclear activity on the cirumnuclear…

宇宙学与河外天体物理 · 物理学 2010-11-02 J. Holt , C. N. Tadhunter , R. Morganti

Gigahertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) sources are compact radio galaxies (RGs), with jets extending up to 20 kpc and ages <10^3 years. They are considered to evolve to Fanaroff-Riley RGs, but the real scenario to…

We present an analysis of the HI absorption in a sample of 101 flux-selected radio AGN (S_1.4 GHz > 50 mJy) observed with the Westerbork Synthesis Radio Telescope (WSRT). HI absorption is detected in 32 galaxies, showing a broad variety of…

星系天体物理 · 物理学 2015-06-23 K. Gereb , F. M. Maccagni , R. Morganti , T. A. Oosterloo

To investigate the impact of radio jets during the formation epoch of their massive host galaxies, we present an analysis of two massive, log(M_stel/ M_sun)~10.6 and 11.3, compact radio galaxies at z=3.5, TNJ0205+2242 and TNJ0121+1320.…

天体物理学 · 物理学 2009-11-13 N. P. H. Nesvadba , M. D. Lehnert , C. De Breuck , A. Gilbert , W. van Breugel

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

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

Our view of the central regions of AGN has been enriched by the discovery of fast and massive outflows of HI and molecular gas. Here we present a brief summary of results obtained for young (and restarted) radio AGN. We find that HI…

星系天体物理 · 物理学 2018-07-20 Raffaella Morganti , Tom Oosterloo , Robert Schulz , Clive Tadhunter , J. B. Raymond Oonk

The study of both neutral and ionized gas in young radio sources is providing key information on the effect the radio plasma has on the ISM of these objects. We present results obtained for the compact radio sources PKS1549-79, 4C12.50 and…

天体物理学 · 物理学 2009-11-07 R. Morganti , C. Tadhunter , T. Oosterloo , J. Holt , A. Tzioumis , K. Wills

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

HI absorption studies yield information on both AGN feeding and feedback processes. This AGN activity interacts with the neutral gas in compact radio sources, which are believed to represent the young or recently re-triggered AGN…

星系天体物理 · 物理学 2017-02-01 M. Glowacki , J. R. Allison , E. M. Sadler , V. A. Moss , S. J. Curran , A. Musaeva , C. Deng , R. Parry , M. C. Sligo

Gas can be used to trace the formation and evolution of galaxies as well as the impact that the nuclear activity has on the surrounding medium. For nearby compact radio sources, we have used observations of neutral hydrogen - that we…

星系天体物理 · 物理学 2009-01-21 R. Morganti , B. Emonts , J. Holt , C. Tadhunter , T. Oosterloo , C. Struve

Young radio AGN are pivotal for our understanding of many of the still-debated aspects of AGN feedback. In this paper we present a study of the interstellar medium in the compact, peaked-spectrum radio galaxy PKSB1934-63 using X-shooter…

星系天体物理 · 物理学 2018-10-03 F. Santoro , M. Rose , R. Morganti , C. Tadhunter , T. A. Oosterloo , J. Holt

Massive outflows of neutral atomic hydrogen (HI) have been observed in absorption in a number of radio galaxies and are considered a signature of AGN feedback. These outflows on kpc-scales have not been investigated in great detail as they…

星系天体物理 · 物理学 2021-03-17 R. Schulz , R. Morganti , K. Nyland , Z. Paragi , E. K. Mahony , T. Oosterloo

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

(Abridged) We present new, intermediate resolution spectra (~4A) of the compact radio source PKS 1345+12. Our spectra clearly show extended line emission (~20kpc) consistent with the asymmetric halo of diffuse emission observed in optical…

天体物理学 · 物理学 2009-11-07 J. Holt , C. N. Tadhunter , R. Morganti
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