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相关论文: Serendipitous Discovery of a BAL QSO at z = 2.169

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We study the transient (i.e. emerging or disappearing) C IV broad absorption line (BAL) components in 50 radio detected QSOs using multi-epoch spectra available in Sloan Digital Sky Survey DR10. We report the detectionof 6 BALQSOs having at…

星系天体物理 · 物理学 2015-11-11 M. Vivek , R. Srianand , N. Gupta

We use the NIRSPEC near-IR spectrometer on Keck II to obtain moderate resolution (R = 1540) spectroscopy that shows conclusively that the C IV emission line in the z = 5.74 quasar SDSSp J104433.04-012502.2 is accompanied by broad,…

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 report the discovery of a Broad Absorption Line (BAL) of \sim 10^4 km s-1 in width in the previously known BL Lac object PKS 0138-097, which we tentatively identified as a Mg II BAL. This is the first detection of a BAL, which is…

宇宙学与河外天体物理 · 物理学 2014-12-24 Zhang Shaohua , Wang Huiyuan , Zhou Hongyan , Wang Tinggui , Jiang Peng

We report kinematic shift and strength variability of C IV broad absorption line (BAL) trough in two high-ionization X-ray bright QSOs SDSS J085551+375752 (at zem ~ 1.936) and SDSS J091127+055054 (at zem ~ 2.793). Both these QSOs have shown…

星系天体物理 · 物理学 2014-06-19 Ravi Joshi , Hum Chand , Raghunathan Srianand , Jhilik Majumdar

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

The existence of BAL outflows in only radio-quiet QSOs was thought to be an important clue to mass ejection and the radio-loud - radio-quiet dichotomy. Recently a few radio-loud BAL QSOs have been discovered at high redshift. We present…

天体物理学 · 物理学 2009-10-31 Beverley J. Wills , W. N. Brandt , A. Laor

We report the detection of a Broad Absorption Line (BAL) outflow in the spectrum of Tol 1037-2703 with three main BALs at 36000, 25300 and 22300~\kms outflow velocities. Although the overall flow is dominated by high ionization lines like…

天体物理学 · 物理学 2009-11-06 R. Srianand , P. Petitjean

We report on the variability of a multi-component broad absorption line (BAL) system observed in the hyper-luminous quasar J1538+0855 at z=3.6. Observations from SDSS, VLT, LBT and Subaru telescopes taken at five different epochs, spanning…

We found a broad absorption line (BAL) outflow in the VLT/UVES spectrum of the quasar SDSS J235702.54-004824.0, in which we identified four subcomponents. We measured the column densities of the ions in one of the subcomponents ($v$ = -1600…

星系天体物理 · 物理学 2022-09-22 Doyee Byun , Nahum Arav , Patrick B. Hall

We present a study of Broad Absorption Line (BAL) quasar outflows that show S IV ?1063 and S IV* ?1073 troughs. The fractional abundance of S IV and C IV peak at similar value of the ionization parameter, implying that they arise from the…

宇宙学与河外天体物理 · 物理学 2015-06-05 Jay P. Dunn , Nahum Arav , Kentaro Aoki , Ashlee Wilkins , Courtney Laughlin , Doug Edmonds , Manuel Bautista

We present a detailed analysis of the Astrophysical Research Consortium 3.5 m telescope spectrum of QSO SDSS J0838+2955. The object shows three broad absorption line (BAL) systems at 22,000, 13,000, and 4900 km s^-1 blueshifted from the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Maxwell Moe , Nahum Arav , Manuel A. Bautista , Kirk T. Korista

We report on the discovery of a peculiar Broad Absorption Line (BAL) quasar identified in our Gaia-assisted survey of red quasars. The systemic redshift of this quasar was difficult to establish due to the absence of conspicuous emission…

We present a multi-epoch spectroscopic study of the broad absorption line (BAL) quasar J115636.82+085628.9 (z(em) = 2.1077), based on five spectra spanning nearly two decades in the observer's frame. This source exhibits remarkable…

星系天体物理 · 物理学 2025-08-05 P. Aromal , R. Srianand , S. C. Gallagher , M. Vivek , P. Petitjean

Broad absorption lines (BALs) in the spectra of quasi-stellar objects (QSOs) originate from outflowing winds along our line of sight; winds are thought to originate from the inner regions of the QSO accretion disk, close to the central…

星系天体物理 · 物理学 2018-09-05 D. De Cicco , W. N. Brandt , C. J. Grier , M. Paolillo , N. Filiz Ak , D. P. Schneider , J. R. Trump

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 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 report the discovery of rapid variations of a high-velocity Mg ii broad absorption line (BAL) trough in the quasar SDSS J133356.02+001229.1 (zem ~ 0.9197). Vivek et al. (2012a) revealed the emergence and subsequent near disappearance of…

星系天体物理 · 物理学 2018-10-17 M. Vivek , R. Srianand , K. S. Dawson

We measure the location and energetics of a SIV BALQSO outflow. This ouflow has a velocity of 10,800 km s$^{-1}$ and a kinetic luminosity of $10^{45.7}$ erg s$^{-1}$, which is 5.2% of the Eddington luminosity of the quasar. From collisional…

星系天体物理 · 物理学 2015-07-02 Carter Chamberlain , Nahum Arav , Chris Benn

(Abridged) We report on HST FOS observations of the double QSO HS 1216+5032 AB (z(A)=1.455; z(B)=1.451, and angular separation theta=9 arcsec). An unusual broad-absorption-line (BAL) system is observed only in the B component: maximum…

天体物理学 · 物理学 2007-05-23 Sebastian Lopez , Hans-Juergen Hagen , Dieter Reimers
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