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相关论文: Low-z MgII Broad Absorption-Line Quasars from the …

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We present nebular emission associated with 198 strong Mg II absorbers at 0.35 $\le z \le$ 1.1 in the fibre spectra of quasars from the Sloan Digital Sky Survey. Measured [O II] luminosities (L$_{[O II]}$) are typical of sub-L$^{\star}$…

星系天体物理 · 物理学 2017-08-23 Ravi Joshi , Raghunathan Srianand , Patrick Petitjean , Pasquier Noterdaeme

First results from a study of high ionization absorption properties in roughly 30 Mg II absorption selected galaxies are presented. We have tested for correlations of Mg II, C IV, Si IV, N V, and O VI equivalent widths with the galaxy…

天体物理学 · 物理学 2008-02-03 Christopher W. Churchill

We have obtained spatially resolved spectra of the z=3.911 triply imaged QSO APM08279+5255 using the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope (HST). We study the line of sight equivalent width (EW)…

We present near-IR, low resolution spectra of eight of the most distant quasars known, with redshifts in the range 4.9<z<6.4. Half of these quasars are characterized by deep, broad and blueshifted absorption features associated with both…

天体物理学 · 物理学 2009-11-10 R. Maiolino , E. Oliva , F. Ghinassi , M. Pedani , F. Mannucci , R. Mujica , Y. Juarez

We report the discovery of five broad-absorption-line (BAL) QSOs in a complete sample of 111 ultraviolet excess (UVX) QSO candidates also detected in the NRAO VLA Sky Survey. All five BAL QSOs, which include two high-ionization BAL QSOs and…

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.…

星系天体物理 · 物理学 2024-02-22 Doyee Byun , Nahum Arav , Maryam Dehghanian , Gwen Walker , Gerard A. Kriss

We present the multiwavelength spectral energy distributions (SEDs) for 65 luminous broad absorption line (BAL) quasars with redshifts $1.55 \lesssim z \lesssim 3.50$ from the Gemini Near Infrared Spectrograph - Distant Quasar Survey…

We present a detailed study of HI and metals for 110 MgII absorption systems discovered at 1.98 <= z <= 5.33 in the infrared spectra of high redshift QSOs. Using new measurements of rest-frame UV lines from optical spectra of the same…

宇宙学与河外天体物理 · 物理学 2015-06-05 Michael S. Matejek , Robert A. Simcoe , Kathy L. Cooksey , Eduardo N. Seyffert

We present new near-infrared (IR) observations of the H$\beta\ \lambda4861$ and MgII $\lambda2798$ lines for 32 luminous quasars with $3.2<z<3.9$ using the Palomar Hale 200 inch telescope and the Large Binocular Telescope. We find that the…

高能天体物理现象 · 物理学 2015-06-23 Wenwen Zuo , Xue-Bing Wu , Xiaohui Fan , Richard Green , Ran Wang , Fuyan Bian

We attempt to characterize the geometry of Broad Absorption Line (BAL) QSOs by studying a low redshift sample of 12 sources. We find that the majority of these sources are Population A quasars as defined in (broad H-beta FWHM > 4000 kms/s;…

天体物理学 · 物理学 2007-05-23 J. W. Sulentic , D. Dultzin-Hacyan , P. Marziani , C. Bongardo , V. Braito , M. Calvani , R. Zamanov

We present a spectropolarimetric survey of 36 broad absorption line quasi-stellar objects (BAL QSOs). The continuum, absorption trough, and emission line polarization of BAL QSOs yield clues about their structure. We confirm that BAL QSOs…

天体物理学 · 物理学 2009-10-31 P. M. Ogle , M. H. Cohen , J. S. Miller , H. D. Tran , R. W. Goodrich , A. R. Martel

Luminous quasars are powerful targets to investigate the role of feedback from supermassive black-holes (BHs) in regulating the growth phases of BHs themselves and of their host galaxies, up to the highest redshifts. Here we investigate the…

Broad Absorption Lines indicate gas outflows with velocities from thousands km/s to about 0.2 the speed of light, which may be present in all quasars and may play a major role in the evolution of the host galaxy. The variability of…

宇宙学与河外天体物理 · 物理学 2015-06-16 D. Trevese , F. G. Saturni , F. Vagnetti , M. Perna , D. Paris , S. Turriziani

A few percent of quasars show strong associated MgII absorption, with velocities (v_off) lying within a few thousand km/s from the quasar systemic redshift. These associated absorption line systems (AALs) are usually interpreted as…

宇宙学与河外天体物理 · 物理学 2015-05-27 Yue Shen , Brice Ménard

In this article, the hydrogen column densities derived from X-ray observations of type II (hidden) quasars and broad absorption line quasars (BALQSOs) are compared. These column densities represent the amount of absorbing material between…

天体物理学 · 物理学 2011-02-11 Brian Punsly

We describe two studies designed to characterize the total column densities, kinetic energies, and acceleration physics of broad absorption line (BAL) outflows in quasars. The first study uses new Chandra X-ray and ground-based rest-frame…

This work presents the results of a Chandra study of 21 broad absorption line (BAL) radio-loud quasars (RLQs). We conducted a Chandra snapshot survey of 12 bright BAL RLQs selected from SDSS/FIRST data and possessing a wide range of radio…

宇宙学与河外天体物理 · 物理学 2009-08-24 B. P. Miller , W. N. Brandt , R. R. Gibson , G. P. Garmire , O. Shemmer

We present a catalog of intervening MgII quasar absorption-line systems in the redshift interval 0.36 <= z <= 2.28. The catalog was built from Sloan Digital Sky Survey Data Release Four (SDSS DR4) quasar spectra. Currently, the catalog…

宇宙学与河外天体物理 · 物理学 2015-05-27 Anna M. Quider , Daniel B. Nestor , David A. Turnshek , Sandhya M. Rao , Eric M. Monier , Anja N. Weyant , Joseph R. Busche

We discuss new high-resolution (6.7 km/s) spectra of the associated absorption lines (AALs) in the radio-loud quasar 3C 191. The measured AALs have ionizations ranging from Mg I to N V, and multi-component profiles that are blueshifted by…

天体物理学 · 物理学 2014-10-13 Frederick W. Hamann , T. A. Barlow , F. C. Chaffee , C. B. Foltz , R. J. Weymann

We present the results of a search for metal absorption lines in the spectra of background QSOs whose sightlines pass close to foreground QSOs. We detect MgII(2796,2803) absorption in Sloan Digital Sky Survey (SDSS) spectra of four z>1.5…