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Feedback from accreting supermassive black holes may regulate galaxy evolution, but statistical evidence linking nuclear winds to kiloparsec-scale cold gas outflows remains limited in the early universe. Here we report statistical evidence…

We have used archival Chandra and XMM-Newton observations of quasars hosting intrinsic narrow UV absorption lines (intrinsic NALs) to carry out an exploratory survey of their X-ray properties. Our sample consists of three intrinsic-NAL…

Astrophysics · Physics 2009-11-13 Toru Misawa , Michael Eracleous , George Chartas , Jane C. Charlton

Broad absorption lines (BALs) found in a significant fraction of quasar spectra identify high-velocity outflows that might be present in all quasars and could be a major factor in feedback to galaxy evolution. Understanding the nature of…

We recently presented radio observations of a large sample of radio-loud broad absorption line (BAL) quasars from the SDSS and FIRST surveys, as well as a well matched sample of unabsorbed quasars, primarily to measure their radio spectral…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 M. A. DiPompeo , M. S. Brotherton , S. L. Cales , J. C. Runnoe

Quasar accretion-disk outflows might play an important role in galaxy evolution, but they are notoriously difficult to study due to line saturation and blending problems in the Ly-alpha forest. We circumvent these problems by constructing…

Astrophysics of Galaxies · Physics 2018-11-07 Fred Hamann , Hanna Herbst , Isabelle Paris , Daniel Capellupo

We isolate a set of quasars that exhibit emergent C iv broad absorption lines (BALs) in their spectra by comparing spectra in the SDSS Data Release 7 and the SDSS/BOSS Data Releases 9 and 10. After visually defining a set of emergent BALs,…

Broad absorption line (BAL) quasars exhibit significant outflows, offering insights into active galactic nuclei (AGN) feedback. While typically associated with high Eddington ratios, BAL quasars also occur in low Eddington ratio regimes,…

Astrophysics of Galaxies · Physics 2025-03-26 M. Vivek , Dominika Wylezalek

We have identified a broad absorption line (BAL) outflow in the HST/STIS spectrum of the quasar QSO B0254-3327B at velocity $v=-3200\text{ km s$^{-1}$}$. The outflow has absorption troughs from ions such as Ne VIII, Na IX, Si XII, and Ne V.…

Astrophysics of Galaxies · Physics 2024-02-22 Doyee Byun , Nahum Arav , Maryam Dehghanian , Gwen Walker , Gerard A. Kriss

We present a statistical analysis of the associated, high ionization narrow absorption line (NAL) systems in a sample of 59 QSOs defined from the HST QSO Absorption Line Key Project. We have compiled the QSO luminosities at 2500 A, 5 GHz,…

We have investigated a sample of 2099 broad absorption line (BAL) quasars with z=1.7-2.2 built from the Sloan Digital Sky Survey Data Release Seven and the Wide-field Infrared Survey. This sample is collected from two BAL quasar samples in…

Astrophysics of Galaxies · Physics 2014-12-24 Shaohua Zhang , Huiyuan Wang , Tinggui Wang , Feijun Xing , Kai Zhang , Hongyan Zhou , Peng Jiang

We statistically study the physical properties of a sample of narrow absorption line (NAL) systems looking for empirical evidences to distinguish between intrinsic and intervening NALs without taking into account any a priori definition or…

We present an analysis of the broad absorption line (BAL) velocity shift that appeared in one of the outflow systems in quasar SDSS J1042+1646. Observations were taken by the Hubble Space Telescope/Cosmic Origin Spectrograph in 2011 and…

Astrophysics of Galaxies · Physics 2020-03-25 Xinfeng Xu , Nahum Arav , Timothy Miller , Gerard A. Kriss , Rachel Plesha

Broad absorption line (BAL) quasars probe the high velocity gas ejected by luminous accreting black holes. BAL variability timescales place constraints on the size, location, and dynamics of the emitting and absorbing gas near the…

Cosmology and Nongalactic Astrophysics · Physics 2012-01-16 Daryl Haggard , Kenza S. Arraki , Paul J. Green , Tom Aldcroft , Scott F. Anderson

Blue-shifted Broad Absorption Lines (BALs) detected in quasar's spectra are indicative of AGN outflows. We show, using 2D hydrodynamical simulations, that disruption of interstellar clouds by a fast AGN wind can lead to formation of cold,…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Meir Zeilig Hess , Amir Levinson , Xinfeng Xu , Nahum Arav

Observational evidence revealing the main mechanisms that accelerate quasar outflows has proven difficult to obtain, due to the complexity of the absorption features that this gas produces in the spectra of the emission sources. We build 36…

Astrophysics of Galaxies · Physics 2019-12-18 Lluís Mas-Ribas , Renate Mauland

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…

Astrophysics of Galaxies · Physics 2018-07-30 S. Komossa , D. W. Xu , A. Y. Wagner

We present results from a comprehensive study of ultrafast outflows (UFOs) detected in a sample of fourteen quasars, twelve of which are gravitationally lensed, in a redshift range of 1.41-3.91, near the peak of the AGN and star formation…

Roughly 10% of all quasars exhibit Broad Absorption Line (BAL) features which appear to arise in material outflowing at high velocity from the active galactic nucleus (AGN). The details of this outflow are, however, very poorly constrained…

Astrophysics · Physics 2009-10-31 Kunegunda E. Belle , Geraint F. Lewis

An analysis of ~19500 narrow (<200 km/s) CIV 1548.2,1550.8 absorbers in ~34000 Sloan Digital Sky Survey quasar spectra is presented. The statistics of the number of absorbers as a function of outflow-velocity shows that in approximately…

Astrophysics of Galaxies · Physics 2015-06-22 Rebecca A. A. Bowler , Paul C. Hewett , James T. Allen , Gary J. Ferland

We have monitored 12 intrinsic narrow absorption lines (NALs) in five quasars and seven mini-broad absorption lines (mini-BALs) in six quasars for a period of 4-12 years (1-3.5 years in the quasar rest-frame). We present the observational…

Astrophysics of Galaxies · Physics 2015-06-22 Toru Misawa , Jane C. Charlton , Michael Eracleous