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相关论文: Multiphase Powerful Outflows Detected in High-z Qu…

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IZw1 is the prototype narrow line quasar. This type of AGNs show a number of common peculiar characteristics whose physical origin is not yet well understood. Here, I review the results of a detailed study by Laor et al. (1997b) of the UV…

天体物理学 · 物理学 2007-05-23 Ari Laor

The growing evidence for energy-conserving outflows in powerful and luminous AGN supports the idea that high-velocity winds launched from the accretion disc evolve systematically after undergoing a shock with the ambient medium and that…

星系天体物理 · 物理学 2018-08-06 Anna Lia Longinotti

We present the stacking analysis of a sample of 48 QSOs at 4.5<z<7.1 detected by ALMA in the [CII] 158 micron line to investigate the presence and the properties of massive, cold outflows traced by broad [CII] wings. We reveal very broad…

星系天体物理 · 物理学 2019-09-25 M. Bischetti , R. Maiolino , S. Carniani. F. Fiore , E. Piconcelli , A. Fluetsch

Bright AGN frequently show ultra-fast outflows (UFOs) with outflow velocities vout ~0.1c. These outflows may be the source of AGN feedback on their host galaxies sought by galaxy formation modellers. The exact effect of the outflows on the…

星系天体物理 · 物理学 2015-06-16 Martin A. Bourne , Sergei Nayakshin

James Webb Space Telescope opens a new window to directly probe luminous quasars powered by billion solar mass black holes in the epoch of reionization and their co-evolution with massive galaxies with unprecedented details. In this paper,…

We exploit the widely-separated images of the lensed quasar SDSS J1029+2623 ($z_{em}$=2.197, $\theta =22^{\prime\prime}\!\!.5$) to observe its outflowing wind through two different sightlines. We present an analysis of three observations,…

Quasar feedback may play a key role in the evolution of massive galaxies. The dust-reddened quasar, F2M110648.35$+$480712 at $z = 0.4352$ is one of the few cases at its redshift that exhibits powerful quasar feedback through bipolar…

Quasar outflows are fundamental components of quasar environments that might play an important role in feedback to galaxy evolution. We report on the emergence of a remarkable new outflow absorption-line system in the quasar PG1411+442…

星系天体物理 · 物理学 2019-06-19 Fred Hamann , Todd M. Tripp , David Rupke , Sylvain Veilleux

We search for velocity changes (i.e., acceleration/deceleration) of narrow absorption lines (NALs) that are intrinsic to the quasars, using spectra of 6 bright quasars that have been observed more than once with 8-10m class telescopes.…

星系天体物理 · 物理学 2019-01-16 Toru Misawa , Michael Eracleous , Jane C. Charlton , Nobunari Kashikawa

We report the first discovery of the emergence of a high-velocity broad-line outflow in a luminous quasar, J105400.40+034801.2 at redshift z ~ 2.1. The outflow is evident in ultraviolet CIV and SiIV absorption lines with velocity shifts v ~…

天体物理学 · 物理学 2009-11-13 F. Hamann , K. F. Kaplan , P. Rodriguez Hidalgo , J. X. Prochaska , S. Herbert-Fort

We present a detailed analysis of the X-ray emission of HS 1700+6416, a high redshift (z=2.7348), luminous quasar, classified as a Narrow Absorption Line (NAL) quasar on the basis of its SDSS spectrum. The source has been observed 9 times…

高能天体物理现象 · 物理学 2015-06-05 G. Lanzuisi , M. Giustini , M. Cappi , M. Dadina , G. Malaguti , C. Vignali , G. Chartas

It is common to assume that all narrow absorption lines (NALs) at extreme high-velocity shifts form in cosmologically intervening gas or galaxies unrelated to quasars. However, previous detailed studies of individual quasars have shown that…

星系天体物理 · 物理学 2021-03-23 Chen Chen , Fred Hamann , Bo Ma

Gas flows between galaxies and the circumgalactic medium (CGM) play a central role in galaxy evolution and can become observable as giant nebulae when illuminated by the quasars. We present an ensemble study of nebulae around 30 UV-luminous…

We present new XMM-Newton and NuSTAR observations of the galaxy merger IRAS F05189-2524 which is classified as an ultra-luminous infrared galaxy (ULIRG) and optical Seyfert 2 at $z$ = 0.0426. We test a variety of spectral models which…

星系天体物理 · 物理学 2020-01-08 Robyn N. Smith , Francesco Tombesi , Sylvain Veilleux , Anne M. Lohfink , Alfredo Luminari

Galaxy formation models invoke the presence of strong feedback mechanisms that regulate the growth of massive galaxies at high redshifts. In this paper we aim to: (1) confirm spectroscopically the redshifts of a sample of massive galaxies…

宇宙学与河外天体物理 · 物理学 2014-04-23 W. Karman , K. I. Caputi , S. C. Trager , O. Almaini , M. Cirasuolo

We investigate the presence and origin of neutral gas outflows and inflows in 13 post-starburst (PSB) and quiescent galaxies at redshifts 1.8 $\leq$ z $\leq$ 4.6, using JWST NIRSpec spectroscopy from the EXCELS survey. NaD absorption…

The prevalence and energetics of quasar feedback is a major unresolved problem in galaxy formation theory. In this paper, we present Gemini Integral Field Unit observations of ionized gas around eleven luminous, obscured, radio-quiet…

宇宙学与河外天体物理 · 物理学 2015-06-16 Guilin Liu , Nadia L. Zakamska , Jenny E. Greene , Nicole P. H. Nesvadba , Xin Liu

Mass outflow rates and loading factors are typically used to infer the quenching potential of galactic-scale outflows. However, these generally rely on observations of a single gas phase which can severely underestimate the total ejected…

星系天体物理 · 物理学 2020-04-22 Guido Roberts-Borsani

Some Active Galactic Nuclei (AGN) host outflows which have the potential to alter the host galaxy's evolution (AGN feedback). These outflows have been linked to enhanced radio emission. Here we investigate the connection between…

We present results from three Suzaku observations of the z=3.91 gravitationally lensed broad absorption line quasar APM 08279+5255. We detect strong and broad absorption at rest-frame energies of <2 keV (low-energy) and 7-12 keV…

宇宙学与河外天体物理 · 物理学 2010-01-15 C. Saez , G. Chartas , W. N. Brandt