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相关论文: A Physical Model of FeLoBALs: Implications for Qua…

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FeLoBALs are a rare class of quasar outflows with low-ionization broad absorption lines (BALs), large column densities, and potentially large kinetic energies that might be important for `feedback' to galaxy evolution. In order to probe the…

星系天体物理 · 物理学 2015-09-09 S. M. McGraw , J. C. Shields , F. W. Hamann , D. M. Capellupo , S. C. Gallagher , W. N. Brandt

The physical properties and dynamical behavior of Broad Absorption Line (BAL) outflows are crucial themes in understanding the connections between galactic centers and their hosts. FeLoBALs (identified with the presence of low-ionization Fe…

We present the first systematic study of 50 low redshift ($0.66 < z < 1.63$) iron low-ionization broad absorption-line quasars (FeLoBALQs) using $SimBAL$ which represents a more than five-fold increase in the number of FeLoBALQs with…

Context. Quasar outflows are often analyzed to determine their ability to contribute to active galactic nucleus (AGN) feedback. We identified a broad absorption line (BAL) outflow in the VLT/UVES spectrum of the quasar SDSS J1321-0041. The…

星系天体物理 · 物理学 2024-02-21 Doyee Byun , Nahum Arav , Mayank Sharma , Maryam Dehghanian , Gwen Walker

Broad absorption line (BAL) features in quasar spectra reveal an unambiguous signature of energetic outflows from central supermassive black holes, and thus BAL quasars are prime targets for investigating the potential process of luminous…

星系天体物理 · 物理学 2020-03-04 Hyunseop Choi , Karen M. Leighly , Donald M. Terndrup , Sarah C. Gallagher , Gordon T. Richards

Photoionization modeling of certain low-ionization broad absorption lines in quasars implies very compact (Delta R~0.01 pc), galaxy-scale (R kpc) absorbers blueshifted by several 1000 km s^-1. While these are likely signatures of quasar…

宇宙学与河外天体物理 · 物理学 2012-01-09 C. -A. Faucher-Giguere

We show for the first time that FBQS J1151+3822 is an iron low-ionization broad absorption line quasar (FeLoBAL QSO), the second-brightest and second-closest known example of this class. He I* and Fe II together act as an effective…

星系天体物理 · 物理学 2014-02-18 Adrian B. Lucy , Karen M. Leighly , Donald M. Terndrup , Matthias Dietrich , Sarah C. Gallagher

We present the optical-near infrared spectral energy distributions (SED) and near infrared variability properties of 30 low-redshift iron low-ionization Broad Absorption Line quasars (FeLoBALQs) and matched samples of LoBALQs and unabsorbed…

Context: The study of quasar outflows is essential in understanding the connection between active galactic nuclei (AGN) and their host galaxies. We analyze the VLT/UVES spectrum of quasar SDSS J0932+0840 and identify several narrow and…

We present Suzaku observations of three iron low-ionization broad absorption line quasars (FeLoBALs). We detect J1723+5553 (3\sigma) in the observed 2--10 keV band, and constrain its intrinsic nh column density to nh > 6\times10^{23} \cmsq…

宇宙学与河外天体物理 · 物理学 2015-05-20 Leah K. Morabito , Xinyu Dai , Karen M. Leighly , Gregory R. Sivakoff , Francesco Shankar

We present mid/far-infrared photometry of nine FeLoBAL QSOs, taken using the Spitzer space telescope. All nine objects are extremely bright in the infrared, with rest-frame 1-1000 micron luminosities comparable to those of Ultraluminous…

天体物理学 · 物理学 2009-11-13 Duncan Farrah , Mark Lacy , Robert Priddey , Colin Borys , Jose Afonso

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…

星系天体物理 · 物理学 2018-11-07 Fred Hamann , Hanna Herbst , Isabelle Paris , Daniel Capellupo

We have observed a dramatic change in the spectrum of the formerly heavily absorbed `overlapping-trough' iron low-ionization broad absorption line (FeLoBAL) quasar FBQS J1408+3054. Over a time span of between 0.6 to 5 rest-frame years, the…

宇宙学与河外天体物理 · 物理学 2015-05-20 Patrick B. Hall , Konstantin Anosov , R. L. White , W. N. Brandt , M. D. Gregg , R. R. Gibson , R. H. Becker , D. P. Schneider

We report the results of analysis of the Hbeta emission-line region of a sample of thirty low-redshift (z<1) iron low-ionization broad absorption line quasars (FeLoBALQs). Eleven of these objects are newly classified as FeLoBALQs. A matched…

We present continued analysis of a sample of low-redshift iron low-ionization broad absorption-line quasars (FeLoBALQs). Choi et al. (2022) presented $SimBAL$ spectral analysis of BAL outflows in 50 objects. Leighly et al. (2022) analyzed…

Quasar outflows have long been recognized as potential contributors to the co-evolution between supermassive black holes (SMBHs) and their host galaxies. The role of outflows in AGN feedback processes can be better understood by placing…

星系天体物理 · 物理学 2018-01-31 S. M. McGraw , J. C. Shields , F. W. Hamann , D. M. Capellupo , H. Herbst

We present the variability study of broad absorption lines (BALs) in a uniformly radio-selected sample of 28 BAL quasars using the archival data from the FIRST Bright Quasar Survey (FBQS) and the Sloan Digital Sky Survey (SDSS), as well as…

星系天体物理 · 物理学 2015-04-17 Shaohua Zhang , Hongyan Zhou , Tinggui Wang , Huiyuan Wang , Xiheng Shi , Bo Liu , Wenjuan Liu , Zhenzhen Li , Shufen Wang

We present near-IR spectroscopy of 22 luminous low-ionization broad absorption line quasars (LoBAL QSOs) at redshift 1.3<z<2.5, with 12 objects at z~1.5 and 10 at z~2.3. The spectra cover the rest-frame H$\alpha$ and H$\beta$ line regions,…

We test a scenario claiming that the broad absorption line (BAL) phenomenon in quasars (QSOs) is not a temporary stage of their life. In this scenario, we see the BAL effect only if the line of sight is within a spatially limited and…

We study the time variability of five Fe Low ionization Broad Absorption Line (FeLoBAL) QSOs using repeated spectroscopic observations with the 2m telescope at IUCAA Girawali observatory (IGO) spanning an interval of upto 10 years. We…

宇宙学与河外天体物理 · 物理学 2015-06-04 M. Vivek , R. Srianand , P. Petitjean , P. Noterdaeme , V. Mohan , A. Mahabal , V. C. Kuriakose
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