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

200 篇论文

We present discovery spectra of a sample of eight lensed galaxies at high redshift, 3.7<z<5.2, selected by their red colors in the fields of four massive clusters: A1689, A2219, A2390, and AC114. Metal absorption lines are detected and…

天体物理学 · 物理学 2009-11-07 Brenda Frye , Tom Broadhurst , Narciso Benitez

The quasar SDSS 0956+5128 exhibits three distinct velocity components with large offsets in emission: the systemic velocity of [O II], [O III] and [Ne III] narrow lines have redshift $z=0.7142$; broad Mg II line is shifted by $-1200$ km…

高能天体物理现象 · 物理学 2023-03-06 V. Rusakov , C. L. Steinhardt , M. Schramm , A. L. Faisst , D. Masters , B. Mobasher , P. Pattarakijwanich

In this paper, we provide new 1 Ms $Chandra$ ACIS spectra of two quasars in the Chandra Deep Field South (CDF-S), which were previously reported to show strong and extremely blueshifted X-ray emission/absorption line features in previous 1…

天体物理学 · 物理学 2009-11-13 Z. Y. Zheng , J. X. Wang

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

Gaseous outflows appear to be a universal property of type-1 and type-2 active galactic nuclei (AGN). The main diagnostic is provided by emission features shifted to higher frequency via the Doppler effect, implying that the emitting gas is…

星系天体物理 · 物理学 2022-03-18 Paola Marziani , Alice Deconto-Machado , Ascension del Olmo

Many theoretical models predict that quasar driven outflows account for the observed quenching of star formation in massive galaxies. There is growing observational evidence for quasar-launched massive outflows at z>6, while the details of…

星系天体物理 · 物理学 2018-10-10 Yueying Ni , Tiziana Di Matteo , Yu Feng , Rupert A. C. Croft , Ananth Tenneti

We present an observational study of 22 broad absorption line quasars (BAL QSOs) at $3\lesssim z \lesssim5$ based on optical/near-IR spectroscopy, aiming to investigate quasar winds and their effects. The near-IR spectroscopy covers the…

星系天体物理 · 物理学 2020-04-29 Weimin Yi , Wenwen Zuo , Jinyi Yang , Feige Wang , John Timlin , Catherine Grier , Xue-Bing Wu , Xiaohui Fan , Jin-Ming Bai

Using data from SDSS, UKIDSS and WISE, we investigate the properties of the high-frequency cutoff to the infrared emission in $\simeq$5000 carefully selected luminous ($L_{bol} \simeq 10^{47}$) type 1 quasars. The strength of $\simeq$2…

星系天体物理 · 物理学 2021-01-18 Matthew J. Temple , Manda Banerji , Paul C. Hewett , Amy L. Rankine , Gordon T. Richards

Quasar outflows may play important role in the evolution of its host galaxy and central black hole. In this paper, we present a detailed study of multiple outflows in the obscured ultra-luminous infrared quasar Q1321+058. The outflows…

宇宙学与河外天体物理 · 物理学 2009-08-24 Tinggui Wang , Hongyan Zhou , Weimin Yuan , Honglin Lu , Xiaobo Dong , Hongguang Shan

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 present the first near-infrared interferometric data of a QSO at z=4. The K-band observations were performed with GRAVITY+ on the VLTI using all four UTs, detecting a differential phase signal that traces the spatially resolved…

We report the discovery of highly reddening and hydrogen Balmer and metastable helium broad absorption lines in the quasar SDSS J145057.28+530007.6, based on the optical and near-infrared spectra taken from the SDSS-III/BOSS and the…

星系天体物理 · 物理学 2018-06-20 Shaohua Zhang , Hongyan Zhou , Xiheng Shi , Xiang Pan , TuoJi , Peng Jiang

Quasars accreting at very high rates are believed to be prime movers of galactic evolution because of their high radiative and mechanical output. The study presented in this paper investigates a sample of six highly accreting quasars at…

星系天体物理 · 物理学 2025-04-29 T. M. Buendia-Rios , P. Marziani , C. A. Negrete , D. Dultzin

Broad absorption line quasars are among the objects presenting the fastest outflows. The launching mechanism itself is not completely understood. Models in which they could be launched from the accretion disk, and then curved and…

星系天体物理 · 物理学 2017-07-12 G. Bruni , K. -H. Mack , F. M. Montenegro-Montes , M. Brienza , J. I. González-Serrano

We report the detection of OH 1667 MHz and wide HI 21cm absorption at $z \sim 0.67$ towards the red quasar 1504+377, with the Green Bank Telescope and the Giant Metrewave Radio Telescope. The HI 21cm absorption extends over a velocity range…

天体物理学 · 物理学 2009-11-13 Nissim Kanekar , Jayaram N. Chengalur

We present a detailed study of the optical and NIR emission and absorption line spectrum of the quasar SDSS J163345.22+512748.4. We discovered on the newly acquired NIR spectrum a highly meta-stable neutral helium broad absorption line…

星系天体物理 · 物理学 2022-04-01 Bo Liu , Hongyan Zhou , Xinwen Shu , Shaohua Zhang , Tuo Ji , Xiang Pan , Peng Jiang

4C 71.07 is a high-redshift blazar whose optical radiation is dominated by quasar-like nuclear emission. We here present the results of a spectroscopic monitoring of the source to study its unbeamed properties. We obtained 24 optical…

星系天体物理 · 物理学 2020-03-11 C. M. Raiteri , J. A. Acosta Pulido , M. Villata , M. I. Carnerero , P. Romano , S. Vercellone

Some cosmological hydrodynamical simulations predict that outflows driven by active galactic nuclei (AGN) play a key role in powering the Ly$\alpha$ nebulae observed around high-redshift quasars. In such simulations, AGN feedback seeded as…

We report on the discovery of a rare case of spatially and kinematically resolved galactic scale outflow at intermediate redshift, based on VLT/MUSE optical integral field spectroscopic observation of the quasar HE 0238$-$1904. This…

星系天体物理 · 物理学 2023-02-08 Qinyuan Zhao , Junfeng Wang

Observational evidence revealing the main mechanisms that accelerate quasar outflows has proven difficult to obtain, due to the complexity of the absorption features that this gas produces in the spectra of the emission sources. We build 36…

星系天体物理 · 物理学 2019-12-18 Lluís Mas-Ribas , Renate Mauland