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相关论文: Blue outliers among intermediate redshift quasars

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The most luminous quasars (with bolometric luminosities are 1E47 erg/s) show a high prevalence of CIV {\lambda}1549 and [OIII]{\lambda}{\lambda}4959,5007 emission line profiles with strong blueshifts. Blueshifts are interpreted as due to…

星系天体物理 · 物理学 2017-09-19 P. Marziani , C. A. Negrete , D. Dultzin , M. L. Martinez-Aldama , A. Del Olmo , M. D'Onofrio , G. M. Stirpe

We perform a systematic study of outflow in the narrow-line region (NLR) of active galactic nuclei (AGNs) at $z\sim0.4-0.8$ basing upon a large sample of $\sim900$ quasars at $z\sim 0.4-0.8$. The sample is extracted from the Sloan Digital…

星系天体物理 · 物理学 2018-01-10 J. Wang , D. W. Xu , J. Y. Wei

We have analyzed the spatially integrated kinematic properties of the ionized gas within the inner r<few kpc in 13 optically selected SDSS type 2 quasars at z~0.3-0.6, using the [OIII]4959,5007 lines. The line profiles show a significant…

宇宙学与河外天体物理 · 物理学 2015-05-30 M. Villar-Martin , A. Humphrey , R. Gonzalez Delgado , L. Colina , S. Arribas

We present a multiwavelength spectral study of the quasar HE0359-3959, which has been identified as an extreme radiating source at intermediate redshift (z=1.5209). Along the spectral range, the different ionic species give information…

We investigate possible factors that drive fast quasar outflows using a sample of 39,249 quasars at median redshift $\langle z \rangle \approx$ 2.17. Unique to this study, the quasar redshifts are re-measured based on the Mg II emission…

星系天体物理 · 物理学 2023-09-07 Jarred Gillette , Fred Hamann

We characterise ionised gas outflows using a large sample of ~330 high-luminosity (45.5 < log(L_bol/erg s^-1) < 49.0), high-redshift (1.5 < z < 4.0) quasars via their [OIII]4960,5008 emission. The median velocity width of the [OIII]…

We present Adaptive Optics assisted near-IR integral field spectroscopic observations of a luminous quasar at $z = 2.4$, previously observed as the first known example at high redshift of large scale quasar-driven outflow quenching star…

星系天体物理 · 物理学 2017-03-22 R. J. Williams , R. Maiolino , Y. Krongold , S. Carniani , G. Cresci , F. Mannucci , A. Marconi

Combining large-area optical quasar surveys with the new far-infrared Herschel-ATLAS Data Release 1, we search for an observational signature associated with the minority of quasars possessing bright far-infrared (FIR) luminosities. We find…

Extremely Red Quasars (ERQs) are thought to represent a brief episode of young quasar and galactic evolution characterized by rapid outflows and obscured growth due to dusty environments. We use new redshift measurements from CO and…

星系天体物理 · 物理学 2023-05-22 Jarred Gillette , Fred Hamann , Marie Wingyee Lau , Serena Perrotta

Aims. Outflows from active galactic nuclei are invoked as the principal feedback process regulating the co-evolution of supermassive black holes and their host galaxies. Because of their multi-phase and multi-scale nature, an exhaustive…

We aim to evaluate the behaviour of our 22 high-redshift (2.2 < z < 3.7) and high-luminosity (47.39 < Lbol < 48.36) quasars in the context of the 4-Dimensional Eigenvector 1. Our approach involves studying quasar physics through…

星系天体物理 · 物理学 2023-01-18 A. Deconto-Machado , A. del Olmo , P. Marziani , J. Perea , G. M. Stirpe

We have observed a sample of 22 luminous quasars, in the range 2.0<z<2.5, at 1.6 microns with the near-infrared (NIR) spectrograph FSPEC on the Multiple Mirror Telescope. Our sample contains 13 radio-loud and 9 radio-quiet objects. We have…

天体物理学 · 物理学 2009-10-31 D. H. McIntosh , H. -W. Rix , M. J. Rieke , C. B. Foltz

We report the discovery of large ionized, [O II] emitting circumgalactic nebulae around the majority of thirty UV luminous quasars at $z=0.4-1.4$ observed with deep, wide-field integral field spectroscopy (IFS) with the Multi-Unit…

We investigate Extremely Red Quasars (ERQs), a remarkable population of heavily-reddened quasars at redshift z$\sim$2 - 3 that might be caught during a short-lived 'blow-out' phase of quasar/galaxy evolution. We perform a near-IR…

星系天体物理 · 物理学 2019-07-31 S. Perrotta , F. Hamann , N. L. Zakamska , R. M. Alexandroff , D. Rupke , D. Wylezalek

We present near-infrared spectra of seven radio-loud quasars with a median redshift of 2.1, five of which were previously known to have Ly alpha nebulae. Extended [OIII]5007 and H alpha emission are evident around six objects, at the level…

天体物理学 · 物理学 2009-10-31 R. J. Wilman , R. M. Johnstone , C. S. Crawford

Outflows from super-massive black holes (SMBHs) play an important role in the co-evolution of themselves, their host galaxies, and the larger scale environments. Such outflows are often characterized by emission and absorption lines in…

We have studied the properties of Seyfert galaxies with high [OIII]5007 blueshifts (`blue outliers'), originally identified because of their strong deviation from the M_BH - sigma relation of normal, narrow-line Seyfert 1 (NLS1) and…

天体物理学 · 物理学 2009-11-13 S. Komossa , D. Xu , H. Zhou , T. Storchi-Bergmann , L. Binette

From Hubble Space Telescope/Cosmic Origins Spectrograph spectra of five quasars, 16 outflows are detected. For 11 outflows, we are able to constrain their distances to the central source (R) and their energetics. In instances of multiple…

星系天体物理 · 物理学 2020-07-22 Timothy R. Miller , Nahum Arav , Xinfeng Xu , Gerard Kriss , Rachel Plesha

We present a study of quasars with very redward asymmetric (RA) ultraviolet (UV) broad emission lines (BELs). An excess of redshifted emission has been previously shown to occur in the BELs of radio loud quasars and is most extreme in…

星系天体物理 · 物理学 2020-11-11 Brian Punsly , Paola Marziani , Marco Berton , Preeti Kharb

While quasar outflows may be quasi-ubiquitous, there are significant differences on a source-by- source basis. These differences can be organized along the 4D Eigenvector 1 sequence: at least at low z, with only Population A sources…

星系天体物理 · 物理学 2016-01-20 P. Marziani , M. A. Martinez Carballo , J. W. Sulentic , A. del Olmo , G. M. Stirpe , D. Dultzin
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