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相关论文: Narrow Absorption Lines Complex. II. Probing the L…

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We discover that some of the broad absorption lines (BALs) are actually a complex of narrow absorption lines (NALs). As a pilot study of this type of BAL, we show this discovery through a typical example in this paper. Utilizing the…

星系天体物理 · 物理学 2017-11-27 Wei-Jian Lu , Ying-Ru Lin

We study the relationship between the broad absorption lines (BALs) that can be decomposed into multiple narrow absorption lines and those that cannot (hereafter Type N and Type S BAL, respectively), based on the analysis of three BAL…

星系天体物理 · 物理学 2019-09-04 Wei-Jian Lu , Ying-Ru Lin

Some fraction of narrow absorption lines are physically associated to the quasar/host-galaxy materials (i.e., intrinsic NALs) like those of BALs and mini-BALs. The relation between these three types of absorption lines has not been…

星系天体物理 · 物理学 2020-09-30 Daisuke Itoh , Toru Misawa , Takashi Horiuchi , Kentaro Aoki

I report the discovery of blueshifted broad absorption line (BAL) troughs in at least six transitions of the Balmer series of hydrogen (Hbeta to H9) and in CaII, MgII and excited FeII in the quasar SDSS J125942.80+121312.6. This is only the…

天体物理学 · 物理学 2008-11-26 Patrick B. Hall

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…

星系天体物理 · 物理学 2015-06-22 Toru Misawa , Jane C. Charlton , Michael Eracleous

Narrow absorption line (NAL) outflows are an important yet poorly understood part of the quasar outflow phenomenon. We discuss one particular NAL outflow that has high speeds, time variability, and moderate ionizations like typical BAL…

宇宙学与河外天体物理 · 物理学 2012-04-18 Fred Hamann , Leah Simon , Paola Rodriguez Hidalgo , Daniel Capellupo

Line locking (LL) of absorption line systems is a clear signature of the dynamical importance of radiation pressure force in driving astrophysical flows, with recent findings suggesting that it may be common in quasars exhibiting multiple…

星系天体物理 · 物理学 2023-03-29 T. R. Lewis , D. Chelouche

We report the discovery of unusual broad absorption lines (BALs) in the bright quasar SDSS J075133.35+134548.3 at z~1, and present a detailed study of BAL and emission lines using the archived and newly obtained optical and NIR…

星系天体物理 · 物理学 2021-05-05 Bo Liu , Hongyan Zhou , Xinwen Shu , Shaohua Zhang , Tuo Ji , Xiang Pan , Peng Jiang

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,…

We present statistical and monitoring results of narrow absorption lines that are physically related to quasars (i.e., intrinsic NALs). We use Keck/HIRES spectra of 37 optically bright quasars at z=2-4, and identify 150 NAL systems that…

天体物理学 · 物理学 2007-05-23 T. Misawa , M. Eracleous , J. C. Charlton , R. Ganguly , D. Tytler , D. Kirkman , N. Suzuki , D. Lubin

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…

天体物理学 · 物理学 2009-10-31 Kunegunda E. Belle , Geraint F. Lewis

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

In this Letter, we report the discovery of a strong correlation between the variability of narrow absorption lines (NALs) and the ionizing continuum from a two-epoch spectra sample of 40 quasars containing 52 variable C iv…

We present a detailed investigation of the variability of 428 C IV and 235 Si IV Broad Absorption Line (BAL) troughs identified in multi-epoch observations of 291 quasars by the Sloan Digital Sky Survey-I/II/III. These observations…

Quasar outflows often consist of two clouds with velocity separations matching the doublet spacings of common UV resonance transitions, a phenomenon known as line-locking, which is commonly observed in quasar spectra. Multiple clouds can be…

星系天体物理 · 物理学 2025-01-14 Chen Chen , Zhicheng He , Weimin Yi , Tuo Ji , Marie Wingyee Lau , Bo Ma

The early stage of massive galaxy evolution often involves outflows driven by a starburst or a central quasar plus cold mode accretion (infall), which adds to the mass build-up in the galaxies. To study the nature of these infall and…

星系天体物理 · 物理学 2020-10-16 Chen Chen , Fred Hamann , Bo Ma , Britt Lundgren , Donald York , Daniel Nestor , Yusra Alsayyad

We report the discovery of disappearance of Mg ii, Al iii, C iv, and Si iv broad absorption lines (BALs) at the same velocity, accompanied by a new Civ BAL emerging at a higher velocity, in the quasar J0827+4252 at z = 2.038. This is the…

星系天体物理 · 物理学 2019-01-23 Weimin Yi , M. Vivek , W. N. Brandt , T. Wang , J. Timlin , N. Filiz Ak , D. P. Schneider , J. P. U. Fynbo , Q. Ni , F. Vito , B. L. Indahl , Sameer

We present an analysis of the variability of broad absorption lines (BALs) in a quasar SDSS J141955.26+522741.1 at $z=2.145$ with 72 observations from the Sloan Digital Sky Survey Data Release 16 (SDSS DR16). The strong correlation between…

星系天体物理 · 物理学 2021-01-12 Qinyuan Zhao , Zhicheng He , Guilin Liu , Tinggui Wang , Hengxiao Guo , Lu Shen , Guobin Mou

This work provides evidence that a large fraction of \ion{C}{IV} narrow absorption lines (NALs) seen along the line of sight to distant quasars are due to accretion disk winds, while also seeking to understand the relationship between NALs…

星系天体物理 · 物理学 2019-08-14 Robert B. Stone , Gordon T. Richards

We report the kinematic shift of the C IV broad absorption line (BAL) in quasar SDSS J120819.29+035559.4 (hereafter J1208+0355). This quasar shows two BAL systems, including a blue component of system A at $\sim$-23500$\,\rm km\,s^{-1}$…

星系天体物理 · 物理学 2020-09-08 Wei-Jian Lu , Ying-Ru Lin
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