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相关论文: An ultra-dense fast outflow in a quasar at z=2.4

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Quasars are galaxies hosting accreting supermassive black holes; due to their brightness, they are unique probes of the early universe. To date, only few quasars have been reported at $z > 6.5$ ($<$800 Myr after the Big Bang). In this work,…

The existence of abundant post-starburst/quiescent galaxies just $\sim$1-2 Gyrs after the Big Bang challenges our current paradigm of galaxy evolution. Cosmological simulations suggest that quasar feedback is likely the most promising…

We present results from three Suzaku observations of the z=3.91 gravitationally lensed broad absorption line quasar APM 08279+5255. We detect strong and broad absorption at rest-frame energies of <2 keV (low-energy) and 7-12 keV…

宇宙学与河外天体物理 · 物理学 2010-01-15 C. Saez , G. Chartas , W. N. Brandt

We have investigated a sample of 5088 quasars from the Sloan Digital Sky Survey Second Data Release in order to determine how the frequency and properties of broad absorptions lines (BALs) depend on black hole mass, bolometric luminosity,…

High velocity outflows from quasars are revealed by the absorption signatures they produce in the spectrum of the quasar. Clues on the nature and origin of these flows are important for our understanding of the dynamics of gas in the…

天体物理学 · 物理学 2009-11-07 R. Srianand , P. Petitjean , C. Ledoux , C. Hazard

We present observations of probable line-of-sight acceleration of a broad absorption trough of C IV in the quasar SDSS J024221.87+004912.6. We also discuss how the velocity overlap of two other outflowing systems in the same object…

天体物理学 · 物理学 2009-06-23 Patrick B. Hall , Sarah I. Sadavoy , Damien Hutsemekers , John E. Everett , Alireza Rafiee

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

Molecular outflows are expected to play a key role in galaxy evolution at high redshift. To study the impact of outflows on star formation at the epoch of reionization, we performed sensitive ALMA observations of OH 119 $\mu$m toward…

We present an analysis of the absorption-line system in the Very Large Telescope/Ultraviolet and Visual Echelle Spectrograph spectrum at a redshift of $z_{\rm a}={3.1448}$ associated with the quasar SDSS J122040.23+092326.96, whose…

星系天体物理 · 物理学 2025-01-03 Qiguo Tian , Lei Hao , Yipeng Zhou , Xiheng Shi , Tuo Ji , Peng Jiang , Lin Lin , Zhenya Zheng , Hongyan Zhou

SDSS J072910.34+333634.3 is a reddened quasar at z=0.96. The archivel Keck/ESI spectrum and our new P200/TripleSpec spectrum reveal an absorption line system in He I*, Ca II H\&K and Na ID. The absorption line system has a width of…

星系天体物理 · 物理学 2016-12-19 Tong Liu , Luming Sun , Xiang Pan , Hongyan Zhou

We report on a variable high-velocity narrow absorption line outflow in the redshift 2.3 quasar J2123-0050. Five distinct outflow systems are detected with velocity shifts from -9710 to -14,050 km/s and CIV 1548,1551 line widths of FWHM =…

宇宙学与河外天体物理 · 物理学 2015-05-19 F. Hamann , N. Kanekar , J. X. Prochaska , M. T. Murphy , S. Ellison , A. L. Malec , N. Milutinovic , W. Ubachs

Substantial evidence in the last few decades suggests that outflows from supermassive black holes (SMBH) may play a significant role in the evolution of galaxies.Large-scale outflows known as warm absorbers (WA) and fast disk winds known as…

We present Keck/ESI long-slit spectroscopy of SBS 1421+511, a system consisting of a quasar at z = 0.276 and an extended source 3" northern to the quasar. The quasar shows a blue-skewed profile of Balmer broad emission lines, which can be…

星系天体物理 · 物理学 2016-02-17 Luming Sun , Hongyan Zhou , Lei Hao , Peng Jiang , Jian Ge , Tuo Ji , Jingzhe Ma , Shaohua Zhang , Xinwen Shu

We present results from X-ray observations of the gravitationally lensed z = 1.51 AGN HS 0810+2554 performed with the Chandra X-ray Observatory and XMM-Newton. Blueshifted absorption lines are detected in both observations at rest-frame…

高能天体物理现象 · 物理学 2016-06-22 G. Chartas , M. Cappi , F. Hamann , M. Eracleous , S. Strickland , M. Giustini , T. Misawa

Galactic outflows driven by rapidly-accreting quasars at high redshift are widely expected to play a key role in the short- and long-term future evolution of their host galaxies. Using new and archival ALMA data, we observed the OH 119um…

Further investigation of data on quasars, especially in the ultraviolet band, yields an amazingly coherent narrative which we present in this paper. Quasars are characterised by strong continuum emission and redshifted emission and…

星系天体物理 · 物理学 2017-12-07 Nimisha G. Kantharia

The early stage of massive galaxy evolution often involves outflows driven by a starburst or a central quasar plus cold mode accretion (infall), which adds to the mass build-up in the galaxies. To study the nature of these infall and…

星系天体物理 · 物理学 2020-10-16 Chen Chen , Fred Hamann , Bo Ma , Britt Lundgren , Donald York , Daniel Nestor , Yusra Alsayyad

We report the emergence of a high velocity, broad absorption line outflow in the luminous quasar Ton 34, at z=1.928. The outflow is detected through an ultraviolet CIV broad absorption line, in a spectrum obtained in January 2006 by the…

宇宙学与河外天体物理 · 物理学 2015-05-20 Y. Krongold , L. Binette , F. Hernandez-Ibarra

We report on the analysis of a ~60 ksec XMM observation of the bright, narrow emission line quasar PG 1211+143. Absorption lines are seen in both EPIC and RGS spectra corresponding to H- and He-like ions of Fe, S, Mg, Ne, O, N and C. The…

天体物理学 · 物理学 2010-04-06 K. A. Pounds , J. N. Reeves , A. R. King , K. L. Page , P. T. O'Brien , M. J. L. Turner

We report the initial result of an adaptive-optics assisted, optical integral-field-unit observation on IRAS04576+0912, the nearest (z=0.039) active galactic nucleus with a prominent blueshift/tail in [O III] emission from a sample of such…