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相关论文: Galaxies at z=3 around Damped Ly-alpha Clouds

200 篇论文

We present 4 new measurements of nitrogen abundances and one upper limit in damped Lyman alpha absorbers (DLAs) obtained by means of high resolution (FWHM \~ 7 km/s) UVES/VLT spectra. In addition to these measurements we have compiled data…

天体物理学 · 物理学 2011-05-23 M. Centurion , P. Molaro , G. Vladilo , C. Peroux , S. A. Levshakov , V. D'Odorico

We present the results of a numerical study of a galactic wind model and its implications on the properties of damped Lyman-alpha absorbers (DLAs) using cosmological hydrodynamic simulations. We vary both the wind strength and the internal…

天体物理学 · 物理学 2008-11-26 Kentaro Nagamine , Arthur M. Wolfe , Lars Hernquist , Volker Springel

We searched quasar spectra from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) for the rare occurrences where a strong damped Lyman-alpha absorber (DLA) blocks the Broad Line Region emission from the quasar and acts as a…

We use a cosmological hydrodynamic simulation of a cold dark matter universe to investigate theoretically the relationship between high redshift galaxies and the Lyman=alpha forest at redshift z=3. Galaxies in the simulation are surrounded…

天体物理学 · 物理学 2016-08-30 Rupert A. C. Croft , Lars Hernquist , Volker Springel , Michael Westover , Martin White

Due to the invention of new powerful instruments in the recent past (e.g. 10m class telescopes) high redshift galaxies are no longer a curiosity. High redshift young star forming galaxies can be effectively discriminated from the much more…

天体物理学 · 物理学 2007-05-23 Eduard Thommes

Using a sample of 92 UV continuum-selected, spectroscopically identified galaxies with <z> = 2.65, all of which have been imaged in the Ly-a line with extremely deep narrow-band imaging, we examine galaxy Ly-a emission profiles to very…

宇宙学与河外天体物理 · 物理学 2015-05-27 C. C. Steidel , M. Bogosavljević , A. E. Shapley , J. A. Kollmeier , N. A. Reddy , D. K. Erb , M. Pettini

We have carried out a high-resolution imaging search for the galaxy associated with the damped Lyman-alpha (DLA) absorber at z=1.859 toward the z_{em}=2.48 quasar QSO 1244+3443, using the HST and the NICMOS. Images were obtained in the…

We report a quantitative study of the escape of Lyman-alpha photons from an inhomogeneous optically thick medium that mimics the structure of damped Lyman-alpha absorbers. Modeling the optically thick disk with 3 components (massive stars…

天体物理学 · 物理学 2007-05-23 O. Puyoo , L. Ben-Jaffel

Lyman break galaxies (LBGs) display a range in structures (from single/compact to clumpy/extended) that is different from typical local star-forming galaxies. Recently, we have introduced a sample of rare, nearby (z<0.3) starbursts that…

宇宙学与河外天体物理 · 物理学 2014-11-20 R. A. Overzier , T. M. Heckman , D. Schiminovich , A. Basu-Zych , T. Goncalves , D. C. Martin , R. M. Rich

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…

天体物理学 · 物理学 2009-10-28 Matthias Bartelmann , Abraham Loeb

We investigate the nature of the physical structures giving rise to damped Lyman alpha absorption systems (DLAS) at high redshift. In particular, we examine the suggestion that rapidly rotating large disks are the only viable explanation…

天体物理学 · 物理学 2009-10-30 Martin G. Haehnelt , Matthias Steinmetz , Michael Rauch

The damped Lyman alpha absorbers (DLAs) in quasar spectra are believed to be the progenitors of present-day disk galaxies. We examine the probability for microlensing of background quasars by stars in their DLAs. Microlensing by an…

天体物理学 · 物理学 2009-10-30 Rosalba Perna , Abraham Loeb

We use medium- and high-resolution spectroscopy of close pairs of quasars to analyze the circumgalactic medium (CGM) surrounding 32 damped Ly$\alpha$ absorption systems (DLAs). The primary quasar sightline in each pair probes an intervening…

Starting from a summary of detection statistics of our recent X-shooter campaign, we review the major surveys, both space and ground based, for emission counterparts of high-redshift damped Ly$\alpha$ absorbers (DLAs) carried out since the…

星系天体物理 · 物理学 2017-06-19 Jens-Kristian Krogager , Palle Møller , Johan P. U. Fynbo , Pasquier Noterdaeme

In an ongoing programme to identify a sample of high z DLA galaxies we have found the long sought for case of a Ly-alpha emitter seen in the centre of a broad DLA trough. This is the predicted `textbook case' of an intervening DLA galaxy if…

天体物理学 · 物理学 2009-11-10 P. Moller , J. P. U. Fynbo , S. M. Fall

We have carried out a high angular resolution near-infrared imaging study of the fields of 6 quasars with 7 strong absorption line systems at z < 0.5, using the Hokupa'a adaptive optics system and the QUIRC near-infrared camera on the…

天体物理学 · 物理学 2008-11-26 Mark R. Chun , Soheila Gharanfoli , Varsha P. Kulkarni , Marianne Takamiya

Damped Ly$\alpha$ absorbers (DLAs) are the highest \HI\ column density (\NHI) absorption line systems detected in the spectra of background quasars. DLAs dominate the neutral gas content of the Universe ($\Omega_{\rm HI}$) and are used to…

We discuss our recent results on the statistical properties of damped Lyman alpha systems (DLAs) at low redshift (z<1.65) (Rao & Turnshek 2000). Contrary to expectations, we found that the cosmological neutral gas mass density as traced by…

天体物理学 · 物理学 2007-05-23 Sandhya M. Rao , David A. Turnshek

To search for low-redshift damped Lyman-alpha (DLA) and sub-DLA quasar absorbers, we have conducted a 21cm absorption survey of radio-loud quasars at small impact parameters to foreground galaxies selected from the Sloan Digital Sky Survey…

宇宙学与河外天体物理 · 物理学 2014-11-20 Sanchayeeta Borthakur , Todd M. Tripp , Min S. Yun , Emmanuel Momjian , Joseph D. Meiring , David V. Bowen , Donald G. York

We present deep GMRT 21cm absorption spectra of 10 damped Lyman-$\alpha$ systems (DLAs), of which 8 are at redshifts $z \ga 1.3$. HI absorption was detected in only one DLA, the $z = 0.5318$ absorber toward PKS 1629+12, which has been…

天体物理学 · 物理学 2008-11-26 Nissim Kanekar , Jayaram N Chengalur