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Related papers: Probing Quasar Outflows with Intrinsic Narrow Abso…

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We use Keck/HIRES spectra of 37 optically bright quasars at z=2-4 to study narrow absorption lines that are intrinsic to the quasars (intrinsic NALs, produced in gas that is physically associated with the quasar central engine). We identify…

Astrophysics · Physics 2009-11-13 T. Misawa , J. C. Charlton , M. Eracleous , R. Ganguly , D. Tytler , D. Kirkman , N. Suzuki , D. Lubin

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

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…

Astrophysics of Galaxies · Physics 2020-09-30 Daisuke Itoh , Toru Misawa , Takashi Horiuchi , Kentaro Aoki

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…

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…

Cosmology and Nongalactic Astrophysics · Physics 2012-04-18 Fred Hamann , Leah Simon , Paola Rodriguez Hidalgo , Daniel Capellupo

We present six new and two previously published high-resolution spectra of the quasar HS 1603+3820 (z_em = 2.542) taken over an interval of 4.2 years (1.2 years in the quasar rest frame). The observations were made with the High-Dispersion…

Astrophysics · Physics 2011-02-11 Toru Misawa , Michael Eracleous , Jane C. Charlton , Nobunari Kashikawa

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

We present a new spectrum of the quasar HS1603+3820 taken 1.28 years (0.36 years in the quasar rest frame) after a previous observation with Subaru+HDS. The new spectrum enables us to search for time variability as an identifier of…

Astrophysics · Physics 2009-11-11 Toru Misawa , Michael Eracleous , Jane C. Charlton , Akito Tajitsu

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,…

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…

Astrophysics of Galaxies · Physics 2019-08-14 Robert B. Stone , Gordon T. Richards

Quasar spectra have a variety of absorption lines whose origins range from energetic winds expelled from the central engines to unrelated, intergalactic clouds. We present multi-epoch, medium resolution spectra of eight quasars at z~2 that…

We present the results of a search for variability in the equivalent widths (EWs) of narrow, associated (Delta v < 5,000 km/s) absorption lines found in the UV spectra of z < 1.5 quasars. The goal of this search was to use variability as a…

Astrophysics · Physics 2009-11-10 J. H. Wise , M. Eracleous , J. C. Charlton , . R. Ganguly

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…

Astrophysics of Galaxies · Physics 2017-11-27 Wei-Jian Lu , Ying-Ru Lin

While narrow absorption lines (NALs) are relatively stable, broad absorption lines (BALs) and mini-BAL systems usually show violent time variability within a few years via a mechanism that is not yet understood. In this study, we examine…

Astrophysics of Galaxies · Physics 2016-05-25 Takashi Horiuchi , Toru Misawa , Tomoki Morokuma , Suzuka Koyamada , Kazuma Takahashi , Hisashi Wada

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 present a catalog of high-velocity CIV $\lambda$ 1548,1551 mini-Broad Absorption Lines (mini-BALs) in the archives of the VLT-UVES and Keck-HIRES spectrographs. We identify high-velocity CIV mini-BALs based on smooth rounded BAL-like…

Astrophysics of Galaxies · Physics 2021-02-03 Chen Chen , Fred Hamann , Bo Ma , Michael Murphy

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…

In the course of a large intervening MgII survey of 25 quasars, the CIV emission lines of six (three radio-loud and three radio-quiet) were observed serendipitously. In four of these six quasars, we detected associated narrow absorption…

We present a census of z(abs) < 2, intrinsic (those showing partial coverage) and associated [z(abs) ~ z(em)] quasar absorption-line systems detected in the Hubble Space Telescope archive of Space Telescope Imaging Spectrograph echelle…

In this paper, we report the line-locking phenomenon of the blended narrow absorption lines (NALs) within trough-like broad absorption lines (BALs) in quasar SDSS J021740.96--085447.9 (hereafter J0217--0854). Utilizing the two-epoch…

Astrophysics of Galaxies · Physics 2018-08-29 Wei-Jian Lu , Ying-Ru Lin
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