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相关论文: Relativistic Outflows in two quasars in the Chandr…

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Broad absorption lines (BALs) in quasar spectra are prominent signatures of high-velocity outflows, which might be present in all quasars and could be a major contributor to feedback to galaxy evolution. Studying the variability in these…

宇宙学与河外天体物理 · 物理学 2015-06-12 Daniel M. Capellupo , Fred Hamann , Joseph C. Shields , Jules P. Halpern , Tom A. Barlow

We report on XMM-Newton spectroscopic observations of the luminous, radio-quiet quasar PDS 456. The hard X-ray spectrum of PDS 456 shows a deep absorption trough (constituting 50% of the continuum) at energies above 7 keV in the quasar rest…

天体物理学 · 物理学 2009-11-10 James Reeves , Paul O'Brien , Martin Ward

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

We report the kinematic shift of the C IV broad absorption line (BAL) in quasar SDSS J120819.29+035559.4 (hereafter J1208+0355). This quasar shows two BAL systems, including a blue component of system A at $\sim$-23500$\,\rm km\,s^{-1}$…

星系天体物理 · 物理学 2020-09-08 Wei-Jian Lu , Ying-Ru Lin

We isolate a set of quasars that exhibit emergent C iv broad absorption lines (BALs) in their spectra by comparing spectra in the SDSS Data Release 7 and the SDSS/BOSS Data Releases 9 and 10. After visually defining a set of emergent BALs,…

Studies of brown dwarf (BD) outflows provide information pertinent to questions on BD formation, as well as allowing outflow mechanisms to be investigated at the lowest masses. Here new observations of the bipolar outflow from the 24…

太阳与恒星天体物理 · 物理学 2015-06-11 Emma Whelan , Tom Ray , Fernando Comeron , Francesca Bacciotti , Patrick Kavanagh

We present a detailed analysis of the X-ray emission of HS 1700+6416, a high redshift (z=2.7348), luminous quasar, classified as a Narrow Absorption Line (NAL) quasar on the basis of its SDSS spectrum. The source has been observed 9 times…

高能天体物理现象 · 物理学 2015-06-05 G. Lanzuisi , M. Giustini , M. Cappi , M. Dadina , G. Malaguti , C. Vignali , G. Chartas

We present an exploratory Chandra ACIS-S3 study of the diffuse component of the Cosmic X-ray Background in the 0.3-7 keV band for four directions at high Galactic latitudes, with emphasis on details of the ACIS instrumental background…

We study the rest-frame optical properties of 74 luminous (L_bol=10^46.2-48.2 erg/s), 1.5<z<3.5 broad-line quasars with near-IR (JHK) slit spectroscopy. Systemic redshifts based on the peak of the [OIII]5007 line reveal that redshift…

星系天体物理 · 物理学 2016-01-27 Yue Shen

In this Letter, the Evans and Koratkar Atlas of Hubble Space Telescope Faint Object Spectrograph Spectra of Active Galactic Nuclei and Quasars is used to study the redward asymmetry in CIV broad emission lines (BELs). It is concluded that…

宇宙学与河外天体物理 · 物理学 2015-05-18 Brian Punsly

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 have obtained optical intermediate resolution spectra (R = 3000) of the narrow-line quasars DMS 0059-0055 and PG 1543+489. The [O III] emission line in DMS 0059-0055 is blueshifted by 880 km/s relative to Hbeta. We also confirm that the…

天体物理学 · 物理学 2009-11-10 Kentaro Aoki , Toshihiro Kawaguchi , Kouji Ohta

We observed 17 optically-selected, radio-quiet high-redshift quasars with the Chandra Observatory ACIS, and detected 16 of them. The quasars have redshift between 3.70 and 6.28 and include the highest redshift quasars known. When compared…

We present unambiguous evidence for a parsec scale wind in the Broad-Line Radio Galaxy (BLRG) 3C 382, the first radio-loud AGN, with $R_{\rm L} = \log_{10}(f_{\rm 5GHz}/f_{4400})>1$, whereby an outflow has been measured with X-ray grating…

高能天体物理现象 · 物理学 2015-05-13 J. N. Reeves , R. M. Sambruna , V. Braito , M. Eracleous

We present the results of a model-independent investigation of the rest-frame UV spectra from a comprehensive sample of $394$ quasars in the redshift range $1.5\leq z \leq 7.5$. We fit the main Broad Emission Lines (BELs) in the rest-frame…

星系天体物理 · 物理学 2019-06-12 Romain A. Meyer , Sarah E. I. Bosman , Richard S. Ellis

Signs of damping wing absorption attenuating the Lyman-$\alpha$ emission line of the first known $z \sim 7$ quasar, ULAS J1120+0641, recently provided exciting evidence of a significantly neutral IGM. This long-awaited signature of…

宇宙学与河外天体物理 · 物理学 2015-07-17 Sarah E. I. Bosman , George D. Becker

We report a synchronized kinematic shift of CIV and SiIV broad absorption lines (BAL) in a high-ionization, radio-loud, and X-ray bright quasar SDSS-J092345+512710 (at $z_{em} \sim 2.1627$). This quasar shows two broad absorption components…

The quasar PDS 456 (at redshift ~0.184) has a prototype ultra-fast outflow (UFO) measured in X-rays. This outflow is highly ionized with relativistic speeds, large total column densities log N_H(cm^-2) > 23, and large kinetic energies that…

星系天体物理 · 物理学 2018-01-24 Fred Hamann , George Chartas , James Reeves , Emanuele Nardini

We report the detection of OVI 1031,1037 and NV 1238,1242 absorption in a system of "mini-broad" absorption lines (mini-BALs) previously reported to have variable CIV 1548,1550 in the quasar PG0935+417. The formation of these lines in an…

宇宙学与河外天体物理 · 物理学 2015-05-19 Paola Rodríguez Hidalgo , Fred Hamann , Patrick Hall

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