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相关论文: The Intrinsically X-ray Weak Quasar PHL 1811. II. …

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We present NuSTAR hard X-ray (3-79 keV) observations of three Type 2 quasars at z ~ 0.4-0.5, optically selected from the Sloan Digital Sky Survey (SDSS). Although the quasars show evidence for being heavily obscured Compton-thick systems on…

Broad emission-line outflows of active galactic nuclei (AGNs) have been proposed for many years but are very difficult to quantitatively study because of the coexistence of the gravitationally-bound and outflow emission. We present detailed…

星系天体物理 · 物理学 2017-02-22 Shaohua Zhang , Hongyan Zhou , Xiheng Shi , Xiang Pan , Ji Wang , Ning Jiang , Tuo Ji , Peng Jiang , Wenjuan Liu , Huiyuan Wang

UVES spectra of the very young (~10^7 years) peculiar B-type star HR 6000 were analyzed in the near-UV and visual spectral regions (3050-9460 A) with the aim to extend to other spectral ranges the study made previously in the UV using IUE…

天体物理学 · 物理学 2009-11-13 F. Castelli , S. Hubrig

We present a high spectral resolution optical spectrum of the bright quasar Q~1037-2704. The large number of absorption systems suggests the presence of an intervening supercluster, but the issue remains controversial.\par We demonstrate…

天体物理学 · 物理学 2007-05-23 Yannick Lespine , Patrick Petitjean

Quasar outflows are fundamental components of quasar environments that might play an important role in feedback to galaxy evolution. We report on the emergence of a remarkable new outflow absorption-line system in the quasar PG1411+442…

星系天体物理 · 物理学 2019-06-19 Fred Hamann , Todd M. Tripp , David Rupke , Sylvain Veilleux

The persistent, low-luminosity neutron star X-ray binary 4U 1812-12 is a potential member of the scarce family of ultra-compact systems. We performed deep photometric and spectroscopic optical observations with the 10.4 m Gran Telescopio…

Steep soft X-ray (0.1-2 keV) quasars share several unusual properties: narrow Balmer lines, strong FeII emission, large and fast X-ray variability, rather steep 2-10 keV spectrum. These intriguing objects have been suggested to be the…

天体物理学 · 物理学 2009-10-30 F. Fiore , G. Matt , M. Cappi , M. Elvis , K. M. Leighly , F. Nicastro , L. Piro , A. Siemiginowska , B. J. Wilkes

We characterize the Ly$\alpha$ halo and absorption systems toward PSO J083+11, a unique $z=6.3401$ weak-line quasar, using Gemini/GNIRS, Magellan/FIRE, and VLT/MUSE data. Strong absorptions by hydrogen and several metal lines (e.g., CII,…

IRAS F11119+3257 is a quasar-dominated Ultra-Luminous InfraRed Galaxy, with a partially obscured narrow-line seyfert 1 nucleus. In this paper, we present the NIR spectroscopy of F11119+3257, in which we find unusual Paschen emission lines,…

星系天体物理 · 物理学 2019-10-14 Xiang Pan , Hongyan Zhou , Wenjuan Liu , Bo Liu , Tuo Ji , Xiheng Shi , Shaohua Zhang , Peng Jiang , Huiyuan Wang , Lei Hao

We report on imaging and spectroscopic observations of the radio-loud, highly polarized quasar PKS 1610-771 (z = 1.71). Our long-slit spectroscopy of the companion 4.55 arcseconds NW of the quasar confirms the stellar nature of this object,…

天体物理学 · 物理学 2007-05-23 F. Courbin , D. Hutsemekers , G. Meylan , P. Magain , S. G. Djorgovski

In this paper we present a broad-band study of the X-ray emission of the blazar PKS1830-211 based on Chandra and Integral observations. Notwithstanding the high redshift (z=2.507), it is a bright X-ray source (F(2-10 keV)~10^{-11} erg…

天体物理学 · 物理学 2009-11-10 A. De Rosa , L. Piro , A. Tramacere , E. Massaro , R. Walter , L. Bassani , A. Malizia , A. J. Bird , A. J. Dean

We analyze archived Chandra and XMM-Newton X-ray observations of 536 Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5) quasars (QSOs) at 1.7 <= z <= 2.7 in order to characterize the relative UV and X-ray spectral properties of QSOs that…

天体物理学 · 物理学 2009-11-13 Robert R. Gibson , W. N. Brandt , Donald P. Schneider

We have analyzed GHRS data of eight CTTS and one WTTS. The GHRS data consists of spectral ranges 40 A wide centered on 1345, 1400, 1497, 1550, and 1900 A. These UV spectra show strong SiIV, and CIV emission, and large quantities of sharp…

天体物理学 · 物理学 2009-11-07 D. R. Ardila , G. Basri , F. M. Walter , J. A. Valenti , C. M. Johns-Krull

We present infrared spectroscopy from the Spitzer Space Telescope at one disk position and two positions at a height of 1 kpc from the disk in the edge-on spiral NGC 891, with the primary goal of studying halo ionization. Our main result is…

天体物理学 · 物理学 2009-11-13 Richard J. Rand , Kenneth Wood , Robert A. Benjamin

We present results on the X-ray spectra of the radio-loud, high-polarization quasar, PKS 1510-089, based on new data obtained using ASCA, and from archival ROSAT data. The X-ray spectrum obtained by ASCA is unusually hard, with the photon…

天体物理学 · 物理学 2009-10-30 K. P. Singh , C. R. Shrader , I. M. George

The neutral hydrogen and the ionized helium absorption in the spectra of quasars are unique probes of structure in the early universe. We present Far-Ultraviolet Spectroscopic Explorer observations of the line of sight to the quasar…

We report the discovery of the faint (V=21.7) quasar QSO03027-0010 at z=2.808 in the vicinity of Q0302-003, one of the few quasars observed with STIS to study intergalactic HeII absorption. Together with another newly discovered QSO at…

天体物理学 · 物理学 2009-11-11 G. Worseck , L. Wisotzki

We report the first mid-IR detection of highly disturbed ionized gas in the ultraluminous infrared galaxy IRAS F00183-7111. The gas, traced by the 12.81um [NeII] and 15.56um [NeIII] lines, spans a velocity range of-3500 to 3000 km/s with…

天体物理学 · 物理学 2011-02-11 H. W. W. Spoon , L. Armus , J. A. Marshall , J. Bernard-Salas , D. Farrah , V. Charmandaris , B. R. Kent

We report NuSTAR observations of a sample of six X-ray weak broad absorption line (BAL) quasars. These targets, at z=0.148-1.223, are among the optically brightest and most luminous BAL quasars known at z<1.3. However, their rest-frame 2…