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Related papers: Molecular QSO Absorption Line Systems

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We discuss simulations of gas at high redshift. We briefly review the methods used and the results for quasar absorption lines. We present gas mass functions and galaxy correlation functions for 5 different cosmological models. Galaxies…

Astrophysics · Physics 2007-05-23 Neal Katz , Lars Hernquist , David H. Weinberg

We propose a three component model consisting of minihalos and galactic halos with embedded thin discs for absorbers producing all the observed classes of intervening quasar absorption line systems. We show that this model, based on CDM…

Astrophysics · Physics 2009-11-06 Snigdha Das , Pushpa Khare , Archana Samantray

Studies of high resolution quasar absorption lines (QALs), arising from gas in local and z < 1.5 galaxies, provide direct probes of the kinematic, chemical, and ionization conditions and evolution of Milky Way-like galaxies. Inferences…

Astrophysics · Physics 2007-05-23 Christopher W. Churchill , Steven S. Vogt

We have obtained low resolution (~20 Angstrom FWHM) slit spectra of 10 quasar candidates located within one degree of the z = 2.181 quasar Q0122-380 with the objective of searching for signs of large scale structure matching the intervening…

Astrophysics · Physics 2007-05-23 R. A. Jansen , P. Jakobsen

Damped Lyman-alpha absorbers are believed to be associated with galactic disks. We show that gravitational lensing can therefore affect the statistics of these systems. First, the magnification bias due to lensing raises faint QSOs above a…

Astrophysics · Physics 2009-10-28 Matthias Bartelmann , Abraham Loeb

We report the first detection of emission line gas within the host galaxies of high redshift QSOs. This was done using narrow-band imaging at the redshifted wavelengths of [O III] and H alpha, using the PUEO adaptive optics camera of the…

Astrophysics · Physics 2009-10-31 J. B. Hutchings , S. L. Morris , D. Crampton

We report a lambda > 1cm search for rotational molecular absorption towards quasars, now possible with the upgraded Australia Telescope Compact Array (ATCA). The targets were PKS 0201+113, PKS 0336-017 and Q 0537-286, where known damped…

Astrophysics · Physics 2009-11-07 S. J. Curran , M. T. Murphy , J. K. Webb , Y. M. Pihlstroem

We used ultraviolet spectra from HST/STIS (R=30,000), together with optical spectra from Keck/HIRES (R=45,000), to study the three MgII-selected absorption systems at z=0.9254, 0.9276, and 0.9342 toward the quasar PG 1206+459. A multi-phase…

Astrophysics · Physics 2007-05-23 Jie Ding

We present spectropolarimetry of 19 confirmed and 4 possible bright, southern broad absorption line (BAL) quasars from the European Southern Observatory (ESO) Very Large Telescope (VLT). A wide range of redshifts is covered in the sample…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Michael A. DiPompeo , Michael S. Brotherton , Carlos De Breuck

We determined C, N and alpha-element relative abundances in the gas surrounding six QSOs at an average redshift of < z > ~ 2.4, by studying six narrow associated absorption systems in UVES high-resolution spectra. We found five systems with…

We report the possible discovery of multiple gravitationally-lensed images of QSOs with angular separations on arcminute scales. The QSOs were selected from the completed 2dF QSO survey as having redshifts and optical colours which are…

Astrophysics · Physics 2011-03-10 L. Miller , A. M. Lopes , R. J. Smith , S. M. Croom , B. J. Boyle , T. Shanks , P. Outram

In this paper we present Monte-Carlo simulations of Lyman alpha absorption systems which originate in galactic haloes, galaxy discs and dark matter (DM) satellites around big central haloes. It is found that for strong Lyman alpha…

Astrophysics · Physics 2009-10-31 W. P. Lin , G. Boerner , H. J. Mo

Recently, convincing evidence was found for extremely large X-ray absorption by column densities $> 10^{23} cm^{-2}$ in broad absorption line quasars. One consequence of this is that any soft X-ray emission from these QSOs would be the…

Astrophysics · Physics 2009-10-31 T. G. Wang , J. X. Wang , W. Brinkmann , M. Matsuoka

Radio-selected samples of quasars with complete optical identifications offer an ideal dataset with which to investigate dust bias associated with intervening absorption systems. Here, we review our work on the Complete Optical and Radio…

Astrophysics · Physics 2009-11-11 Sara L. Ellison

We review the ongoing debate about the relationship between low redshift Lyman Alpha absorbers and luminous galaxies. In particular, we discuss the difficulty of `assigning' a particular absorber to a particular galaxy, and consider methods…

Astrophysics · Physics 2007-05-23 Simon L. Morris , Buell Jannuzi , Ray Weymann

We present results of an ongoing program to study the gaseous extent of galaxies and the origin of QSO absorption line systems. For \lya absorption systems, we find that absorption equivalent width depends strongly on galaxy impact…

Astrophysics · Physics 2016-08-15 H. -W. Chen , K. M. Lanzetta , J. K. Webb , X. Barcons , A. Fernández-Soto

We present a new measurement of the space density of high redshift (3.0<z<4.5), X-ray selected QSOs obtained by exploiting the deep and uniform multiwavelength coverage of the COSMOS survey. We have assembled a statistically large (40…

We present the discovery of strong Balmer line absorption in H$\alpha$ to H$\gamma$ in two luminous low-ionization broad absorption line quasars (LoBAL QSOs) at z~1.5, with black hole masses around $10^{10}$ $M_\odot$ from near-IR…

Astrophysics of Galaxies · Physics 2018-02-21 Andreas Schulze , Toru Misawa , Wenwen Zuo , Xue-Bing Wu

In hierarchical cosmogonies at redshift three the matter content of a typical present-day galaxy is dispersed over several individual clumps embedded in sheet-like structures, often aligned along filaments. We have used hydrodynamical…

Astrophysics · Physics 2016-08-30 Michael Rauch , Martin G. Haehnelt , Matthias Steinmetz

We present spectra of QSOs 1343+266 A B, covering Ly-beta to C~IV emission at 2\AA~resolution, and find further evidence that this system is not gravitationally lensed. We see, however, a large number of Ly-alpha and some C~IV absorption…

Astrophysics · Physics 2009-10-22 Arlin P. S. Crotts , Jill Bechtold , Yihu Fang , Robert C. Duncan
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